NAME the Pipe Nebula , the SIMBAD biblio

NAME the Pipe Nebula , the SIMBAD biblio (405 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.06.14CEST07:20:07

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Title First 3 Authors
1995MNSSA..54...72. 127 0 The nomenclature of deep-sky objects.
1999PASJ...51..871O 72 T                   29 76 NANTEN observations of the Pipe Nebula: a filamentary massive dark cloud with very low star-formation activity. ONISHI T., KAWAMURA A., ABE R., et al.
2002A&A...385..909T 2 11 89 Statistical study of C18O dense cloud cores and star formation. TACHIHARA K., ONISHI T., MIZUNO A., et al.
2004MmSAI..75..509F 6 4 Observations of the darkest regions in the sky: X-ray shadowing by the Bok globule Barnard 68. FREYBERG M.J., BREITSCHWERDT D. and ALVES J.
2004BaltA..13..349P 21 4 The slow mode of star formation: A critical appraisal. PALLA F.
2005ApJ...634..476Y 73 75 High-mass cloud cores in the η Carinae giant molecular cloud. YONEKURA Y., ASAYAMA S., KIMURA K., et al.
2006A&A...453..635M viz 17 15 522 Modelling the Galactic interstellar extinction distribution in three dimensions. MARSHALL D.J., ROBIN A.C., REYLE C., et al.
2006A&A...454..781L 123 T K                 9 204 2MASS wide field extinction maps. I.
The Pipe nebula.
2007ApJ...655..364B 37 58 The Spitzer c2d survey of nearby dense cores. IV. Revealing the embedded cluster in B 59. BROOKE T.Y., HUARD T.L., BOURKE T.L., et al.
2007A&A...462L..17A viz 35 6 429 The mass function of dense molecular cores and the origin of the IMF. ALVES J., LOMBARDI M. and LADA C.J.
2007ApJ...664..357R 3 8 60 The infrared extinction law at extreme depth in a dark cloud core. ROMAN-ZUNIGA C.G., LADA C.J., MUENCH A., et al.
2007MNRAS.379...57C 42           X         1 5 54 Clump lifetimes and the initial mass function. CLARK P.C., KLESSEN R.S. and BONNELL I.A.
2007A&A...470..597A 1820 T K A S   X C       46 103 43 An accurate determination of the distance to the
Pipe nebula.
2007ApJ...665..457A 17 25 The dynamical state of the starless dense core FeSt 1-457: a pulsating globule? AGUTI E.D., LADA C.J., BERGIN E.A., et al.
2007PASP..119..855W 1 48 140 The James Clerk Maxwell Telescope legacy survey of nearby star-forming regions in the Gould belt. WARD-THOMPSON D., DI FRANCESCO J., HATCHELL J., et al.
2007ApJ...668..906M viz 40 47 Massive clumps in the NGC 6334 star-forming region. MUNOZ D.J., MARDONES D., GARAY G., et al.
2007MNRAS.381L..40D 46           X         1 2 36 The origin of the Arches stellar cluster mass function. DIB S., KIM J. and SHADMEHRI M.
2007A&A...475..263F 11 12 Physical characteristics of a dark cloud in an early stage of star formation toward NGC 7538. An outer Galaxy infrared dark cloud? FRIESWIJK W.W.F., SPAANS M., SHIPMAN R.F., et al.
2007ARA&A..45..339B 12 30 762 Cold dark clouds : the initial conditions for star formation. BERGIN E.A. and TAFALLA M.
2007ApJ...671.1820M 735 T   A S O X C       17 13 33 The nature of the dense core population in the pipe nebula: core and cloud kinematics from C18O observations. MUENCH A.A., LADA C.J., RATHBORNE J.M., et al.
2008ApJ...672..410L 483 T   A     X C       11 11 192 The nature of the dense core population in the Pipe nebula: thermal cores under pressure. LADA C.J., MUENCH A.A., RATHBORNE J., et al.
2008A&A...477..823G 41           X         1 7 44 The relationship between the prestellar core mass function and the stellar initial mass function. GOODWIN S.P., NUTTER D., KROUPA P., et al.
2008ApJS..174..396R 1342 T   A     X C       34 10 38 The nature of the dense core population in the pipe nebula: a survey of NH3, CCS, and HC5 N molecular line emission. RATHBORNE J.M., LADA C.J., MUENCH A.A., et al.
2008ApJ...674..316H 64           X         1 3 160 Cooling, gravity, and geometry: flow-driven massive core formation. HEITSCH F., HARTMANN L.W., SLYZ A.D., et al.
2008ApJ...674..831F 38           X         1 9 9 Hunting galaxies to (and for) extinction. FOSTER J.B., ROMAN-ZUNIGA C.G., GOODMAN A.A., et al.
2008MNRAS.386.1069W 41           X         1 8 55 Molecular line mapping of the giant molecular cloud associated with RCW 106 - II. Column density and dynamical state of the clumps. WONG T., LADD E.F., BRISBIN D., et al.
2008ApJ...679..481P 7 15 230 CO isotopologues in the Perseus molecular cloud complex: the X-factor and regional variations. PINEDA J.E., CASELLI P. and GOODMAN A.A.
2008ApJ...679..552S 192           X         5 5 40 On the evolution of the dense core mass function. SWIFT J.J. and WILLIAMS J.P.
2008ApJ...681..365E 114           X         3 20 78 On the constancy of the characteristic mass of young stars. ELMEGREEN B.G., KLESSEN R.S. and WILSON C.D.
2008A&A...486L..13A 937 T K A S   X C       22 5 103 Optical polarimetry toward the
Pipe nebula: revealing the importance of the magnetic field.
2008ApJ...682.1095B 151           X C       3 6 9 The damping rates of embedded oscillating starless cores. BRODERICK A.E., NARAYAN R., KETO E., et al.
2008ApJ...684.1240E viz 226           X         6 220 274 The mass distribution and lifetime of prestellar cores in Perseus, Serpens, and Ophiuchus. ENOCH M.L., EVANS II N.J., SARGENT A.I., et al.
2008A&A...489..143L 453           X C       11 33 99 2MASS wide field extinction maps. II. The Ophiuchus and the Lupus cloud complexes. LOMBARDI M., LADA C.J. and ALVES J.
2008MNRAS.390..807C 339     A D     X C F     8 12 3 The directional analysis of star clusters. CARTWRIGHT A. and WHITWORTH A.P.
2008ApJ...687..340M 113           X         3 15 28 Protostar mass due to infall and dispersal. MYERS P.C.
2008ApJ...687..354N 481     A S   X C       11 13 172 Magnetically regulated star formation in three dimensions: the case of the Taurus Molecular Cloud complex. NAKAMURA F. and LI Z.-Y.
2008PASP..120.1193G 30 3 Molecular tracers of embedded star formation in Ophiuchus. GURNEY M., PLUME R. and JOHNSTONE D.
2009ApJ...690.1659R 76           X         2 9 5 The dense ring in the Coalsack: the merging of two subsonic flows? RATHBORNE J.M., LADA C.J., WALSH W., et al.
2009A&A...493..735L 393           X C       9 3 87 Nicest, a near-infrared color excess method tailored to small-scale structures. LOMBARDI M.
2009MNRAS.392..341C 205       D     X   F     5 9 10 Analysing the structure of elongated star clusters. CARTWRIGHT A. and WHITWORTH A.P.
2009ApJ...692...91G 157           X         4 15 168 The "True" column density distribution in star-forming molecular clouds. GOODMAN A.A., PINEDA J.E. and SCHNEE S.L.
2009NewA...14..221B 77           X         2 9 24 Nonlinear evolution of gravitational fragmentation regulated by magnetic fields and ambipolar diffusion. BASU S., CIOLEK G.E. and WURSTER J.
2009ApJ...691.1560I viz 114           X         3 22 25 A survey of dense cores in the Orion B cloud. IKEDA N., KITAMURA Y. and SUNADA K.
2009ApJS..181..321E viz 38           X         1 1054 1239 The Spitzer c2d legacy results: star-formation rates and efficiencies: evolution and lifetimes. EVANS N.J., DUNHAM M.M., JORGENSEN J.K., et al.
2009ApJ...695.1308B 194           X C F     3 2 21 The inevitable future of the starless core Barnard 68. BURKERT A. and ALVES J.
2009ApJ...696..298F viz 117           X         3 9 61 Dense cores in Perseus: the influence of stellar content and cluster environment. FOSTER J.B., ROSOLOWSKY E.W., KAUFFMANN J., et al.
2009A&A...497..399K 1053     A   O X C       27 2 31 The fidelity of the core mass functions derived from dust column density data. KAINULAINEN J., LADA C.J., RATHBORNE J.M., et al.
2009ApJ...697.1457F 152           X         4 48 75 The initial conditions of clustered star formation. I. NH3Observations of dense cores in Ophiuchus. FRIESEN R.K., DI FRANCESCO J., SHIRLEY Y.L., et al.
2009ApJ...698..324R viz 38           X         1 337 53 Detection of structure in infrared-dark clouds with Spitzer: characterizing star formation in the molecular ring. RAGAN S.E., BERGIN E.A. and GUTERMUTH R.A.
2009MNRAS.395.1640R 40           X         1 15 79 The structure of molecular clouds - I. All-sky near-infrared extinction maps. ROWLES J. and FROEBRICH D.
2009MNRAS.396..830S 43           X         1 6 60 Fragmentation in molecular clouds and its connection to the IMF. SMITH R.J., CLARK P.C. and BONNELL I.A.
2009ApJ...699..585H 356       D     X         10 147 62 A search for carbon-chain-rich cores in dark clouds. HIROTA T., OHISHI M. and YAMAMOTO S.
2009ApJ...699..742R viz 1565 T   A D S   X C F     38 3 69 Dense cores in the
Pipe Nebula: an improved core mass function.
2008BaltA..17..253S 37 22 2MASS two-color interstellar reddening lines in the inner galaxy. STRAIZYS V. and LAUGALYS V.
2009ApJ...700.1541R 76           X         2 19 10 2MASS J17112318-2724315: a deeply embedded low-mass protostellar system in the B59 molecular cloud. RIAZ B., MARTIN E.L., BOUY H., et al.
2009ApJ...700.1609M 117           X C       2 46 333 Filamentary structure of star-forming complexes. MYERS P.C.
2009ApJ...702..352L 154           X C       3 13 73 The structure of a low-metallicity giant molecular cloud complex. LEROY A.K., BOLATTO A., BOT C., et al.
2009ApJ...702.1428H 57           X         1 4 154 Analytical theory for the initial mass function. II. Properties of the flow. HENNEBELLE P. and CHABRIER G.
2009A&A...503..859B viz 212     A     X         6 14 23 Multiple low-turbulence starless cores associated with intermediate- to high-mass star formation. BEUTHER H. and HENNING T.
2009ApJ...703...52L 76           X         2 62 118 The California molecular cloud. LADA C.J., LOMBARDI M. and ALVES J.F.
2009MNRAS.397L..36G 41           X         1 2 15 What does a universal initial mass function imply about star formation? GOODWIN S.P. and KOUWENHOVEN M.B.N.
2009ApJ...704..183R 554 T   A     X         14 8 21 High resolution near-infrared survey of the
Pipe Nebula. I. A deep infrared extinction map of Barnard 59.
2009ApJ...704..292F 1387 T   A S   X C       34 48 32 A Spitzer census of star formation activity in the
Pipe Nebula.
2009ApJ...704..531K viz 15       D     X         1 180 142 The coevality of young binary systems. KRAUS A.L. and HILLENBRAND L.A.
2009ApJ...704.1735H 409 T   A S   X         9 4 59 Gravitational collapse and filament formation: comparison with the Pipe Nebula. HEITSCH F., BALLESTEROS-PAREDES J. and HARTMANN L.
2009ApJ...707...89G viz 41           X         1 8 52 Mid-infrared extinction and its variation with galactic longitude. GAO J., JIANG B.W. and LI A.
2009ApJ...706.1341M 78           X         2 5 25 On the distribution of protostar masses. MYERS P.C.
2009ApJ...707.1824N viz 114           X         3 154 48 BLAST: the mass function, lifetimes, and properties of intermediate mass cores from a 50 deg2 submillimeter galactic survey in Vela (l∼265°). NETTERFIELD C.B., ADE P.A.R., BOCK J.J., et al.
2009ApJ...707.1836O viz 38           X         1 153 22 The BLAST survey of the Vela molecular cloud: physical properties of the dense cores in Vela-D. OLMI L., ADE P.A.R., ANGLES-ALCAZAR D., et al.
2010ApJ...710..470D 45           X         1 10 152 Evolutionary signatures in the formation of low-mass protostars. II. Toward reconciling models and observations. DUNHAM M.M., EVANS N.J., TEREBEY S., et al.
2009A&A...508L..35K 98       D   O X         3 25 355 Probing the evolution of molecular cloud structure. From quiescence to birth. KAINULAINEN J., BEUTHER H., HENNING T., et al.
2010A&A...509A..44M 38           X         1 29 14 A method to determine distances to molecular clouds using near-IR photometry. MAHESWAR G., LEE C.W., BHATT H.C., et al.
2010PASP..122..224S 15       D               2 8 9 Discerning the form of the dense core mass function. SWIFT J.J. and BEAUMONT C.N.
2010A&A...510A.110H 42           X         1 2 17 The thermodynamics of molecular cloud fragmentation. Star formation under non-Milky way conditions. HOCUK S. and SPAANS M.
2010ApJ...712.1137K 41           X         1 8 55 The mass-size relation from clouds to cores. I. A new probe of structure in molecular clouds. KAUFFMANN J., PILLAI T., SHETTY R., et al.
2010A&A...512A..44L 153           X         4 54 39 Searching for chameleon-like scalar fields with the ammonia method. LEVSHAKOV S.A., MOLARO P., LAPINOV A.V., et al.
2010A&A...512A..67L 38           X         1 59 112 2MASS wide field extinction maps. III. The Taurus, Perseus, and California cloud complexes. LOMBARDI M., LADA C.J. and ALVES J.
2010A&A...512A..81F 59         O X         1 15 657 Comparing the statistics of interstellar turbulence in simulations and observations. Solenoidal versus compressive turbulence forcing. FEDERRATH C., ROMAN-DUVAL J., KLESSEN R.S., et al.
2010ApJ...716..167M 39           X         1 10 34 The protostellar mass function. McKEE C.F. and OFFNER S.S.R.
2010ApJ...716..433K 956     A D     X C       25 16 122 The mass-size relation from clouds to cores. II. Solar neighborhood clouds. KAUFFMANN J., PILLAI T., SHETTY R., et al.
2010ApJ...716..893P viz 76           X         2 42 31 Magnetic field structures and turbulent components in the star-forming molecular clouds OMC-2 and OMC-3. POIDEVIN F., BASTIEN P. and MATTHEWS B.C.
2010ApJ...718L..32S 38           X         1 33 23 "Starless" super-jeans cores in four Gould Belt clouds. SADAVOY S.I., DI FRANCESCO J. and JOHNSTONE D.
2010MNRAS.405..401D 115           X         3 24 63 The IMF of stellar clusters: effects of accretion and feedback. DIB S., SHADMEHRI M., PADOAN P., et al.
2010MNRAS.405.1431A 80           X         2 6 57 Collision between dissimilar clouds: stability of the bow-shock, and the formation of pre-stellar cores. ANATHPINDIKA S.V.
2010MNRAS.406..505S 38           X         1 40 2 A near-infrared variability study in the cloud IC1396W: low star-forming efficiency and two new eclipsing binaries. SCHOLZ A., FROEBRICH D., DAVIS C.J., et al.
2010ApJ...719..691F 1281 T   A     X C       32 43 14 Nothing to hide: an X-ray survey for young stellar objects in the Pipe nebula. FORBRICH J., POSSELT B., COVEY K.R., et al.
2010ApJ...721..493B 38           X         1 5 9 The evolution of cloud cores and the formation of stars. BRODERICK A.E. and KETO E.
2010ApJ...721.1206C 76           X         2 89 44 Spitzer view of young massive stars in the Large Magellanic Cloud H II complexes. II. N 159. CHEN C.-H.R., INDEBETOUW R., CHU Y.-H., et al.
2010A&A...516A.113L 38           X         1 17 12 Searching for spatial variations of alpha2/µ in the Milky Way. LEVSHAKOV S.A., MOLARO P. and REIMERS D.
2010MNRAS.407.1981G 38           X         1 41 28 Have protoplanetary discs formed planets{quest}. GREAVES J.S. and RICE W.K.M.
2010ApJ...722..971C 519     A     X C       13 78 60 The age, stellar content, and star formation timescale of the B59 dense core. COVEY K.R., LADA C.J., ROMAN-ZUNIGA C., et al.
2010ApJ...723L...7K 89           X         2 7 187 How many infrared dark clouds can form massive stars and clusters? KAUFFMANN J. and PILLAI T.
2010ApJ...723..146F 2160 T K A     X C       55 24 68 Detailed interstellar polarimetric properties of the Pipe Nebula at core scales. FRANCO G.A.P., ALVES F.O. and GIRART J.M.
2010A&A...519L...7L 169       D       C F     4 27 97 Larson's third law and the universality of molecular cloud structure. LOMBARDI M., ALVES J. and LADA C.J.
2010ApJ...723.1065O 38           X         1 6 4 The BLAST survey of the Vela molecular cloud: dynamical properties of the dense cores in Vela-D. OLMI L., ANGLES-ALCAZAR D., DE LUCA M., et al.
2010ApJ...723.1665F 1510 T K A S   X C       37 15 26 Young starless cores embedded in the magnetically dominated Pipe nebula. FRAU P., GIRART J.M., BELTRAN M.T., et al.
2010ApJ...724..687L 206           X         5 19 584 On the star formation rates in molecular clouds. LADA C.J., LOMBARDI M. and ALVES J.F.
2010A&A...520A..17K 43           X         1 25 271 Accretion-driven turbulence as universal process: galaxies, molecular clouds, and protostellar disks. KLESSEN R.S. and HENNEBELLE P.
2010MNRAS.408.1089T 42           X         1 4 36 Do lognormal column-density distributions in molecular clouds imply supersonic turbulence ? TASSIS K., CHRISTIE D.A., URBAN A., et al.
2010ApJ...725.1327S 267           X         7 57 43 Star formation in the Taurus filament L 1495: from dense cores to stars. SCHMALZL M., KAINULAINEN J., QUANZ S.P., et al.
2010ApJ...725.2232R viz 1359 T   A S   X C       33 12 31 Deep near-infrared survey of the Pipe nebula. II. Data, methods, and dust extinction maps. ROMAN-ZUNIGA C.G., ALVES J.F., LADA C.J., et al.
2010A&A...524A..91M 114           X         3 35 12 Physical properties of dense cores in Orion B9. MIETTINEN O., HARJU J., HAIKALA L.K., et al.
2011ApJ...726...46N 154           X         4 39 35 The molecular outflows in the ρ Ophiuchi main cloud: implications for turbulence generation. NAKAMURA F., KAMADA Y., KAMAZAKI T., et al.
2011ApJ...728..104S viz 54       D     X         2 897 31 Optical polarization mapping toward the interface between the Local Cavity and Loop I. SANTOS F.P., CORRADI W. and REIS W.
2011ApJ...728..123K 46           X         1 2 32 Formation of collapsing cores in subcritical magnetic clouds: three-dimensional magnetohydrodynamic simulations with ambipolar diffusion. KUDOH T. and BASU S.
2011MNRAS.411.2067L 38           X         1 10 17 Evidence for dynamically important magnetic fields in molecular clouds. LI H.-B., BLUNDELL R., HEDDEN A., et al.
2011A&A...527A.145B viz 115           X         3 102 65 The end of star formation in Chamaeleon I? A LABOCA census of starless and protostellar cores. BELLOCHE A., SCHULLER F., PARISE B., et al.
2011ApJ...731....8K viz 78           X         2 143 291 Mapping the shores of the brown dwarf desert. II. Multiple star formation in Taurus-Auriga. KRAUS A.L., IRELAND M.J., MARTINACHE F., et al.
2011A&A...528A..50D 39           X         1 15 52 Was a cloud-cloud collision the trigger of the recent star formation in Serpens? DUARTE-CABRAL A., DOBBS C.L., PERETTO N., et al.
2011ApJ...732..101I viz 154           X         4 23 8 Similarity between the C18O (J = 1-0) core mass function and the initial mass function (IMF) in the S140 region. IKEDA N. and KITAMURA Y.
2011MNRAS.412.1755L 116           X C       2 4 10 Forming protostars in molecular clouds with shocked envelope expansion and core collapse. LOU Y.-Q. and GAO Y.
2011A&A...529A...1S 55       D     X         2 50 109 The link between molecular cloud structure and turbulence. SCHNEIDER N., BONTEMPS S., SIMON R., et al.
2011NewAR..55...23V 15       D               1 220 6 Magnetic fields in the nearby Universe, as observed in solar and planetary realms, stars, and interstellar starforming nurseries. VALLEE J.P.
2011A&A...530A..64K 208       D     X         6 26 79 Probing the evolution of molecular cloud structure. II. From chaos to confinement. KAINULAINEN J., BEUTHER H., BANERJEE R., et al.
2011A&A...530A.118P viz 39           X         1 52 107 Probing the initial conditions of high-mass star formation. II. Fragmentation, stability, and chemistry towards high-mass star-forming regions G29.96-0.02 and G35.20-1.74. PILLAI T., KAUFFMANN J., WYROWSKI F., et al.
2011AJ....142...33A 38           X         1 43 13 Infrared and optical polarimetry around the low-mass star-forming region NGC 1333 IRAS 4A. ALVES F.O., ACOSTA-PULIDO J.A., GIRART J.M., et al.
2011ApJS..194...43P viz 38           X         1 233 62 The Spitzer survey of interstellar clouds in the Gould Belt. III. A multi-wavelength view of Corona Australis. PETERSON D.E., CARATTI O GARATTI A., BOURKE T.L., et al.
2011ApJ...735...51M 269           X         7 21 14 Mass distributions of stars and cores in young groups and clusters. MICHEL M., KIRK H. and MYERS P.C.
2011ApJ...735...82M 38           X         1 15 24 Filamentary condensations in a young cluster. MYERS P.C.
2011ApJ...736..149G 38           X         1 35 25 Galactic H2 CO densitometry. I. Pilot survey of ultracompact H II regions and methodology. GINSBURG A., DARLING J., BATTERSBY C., et al.
2011A&A...531A..26B viz 38           X         1 13 14 High-mass star formation at high luminosities: W31 at >106 L☉. BEUTHER H., LINZ H., HENNING Th., et al.
2011ApJ...738..152S 38           X         1 16 3 Prestellar cores in the Coalsack. SAUL M., CUNNINGHAM M., RATHBORNE J., et al.
2011ApJ...739...25M 44           X         1 15 181 Lifting the dusty veil with near- and mid-infrared photometry. I. Description and applications of the Rayleigh-Jeans color excess method. MAJEWSKI S.R., ZASOWSKI G. and NIDEVER D.L.
2011ApJS..196...12B viz 38           X         1 489 50 The Galactic Census of High- and Medium-mass Protostars. I. Catalogs and first results from Mopra HCO+ maps. BARNES P.J., YONEKURA Y., FUKUI Y., et al.
2011MNRAS.416..710F 64           X         1 2 106 Does external pressure explain recent results for molecular clouds? FIELD G.B., BLACKMAN E.G. and KETO E.R.
2011MNRAS.416..783P 39           X         1 4 12 Volume density thresholds for overall star formation imply mass–size thresholds for massive star formation. PARMENTIER G., KAUFFMANN J., PILLAI T., et al.
2011ApJ...743...54T viz 192           X         5 172 15 Correlating the interstellar magnetic field with protostellar jets and its sources. TARGON C.G., RODRIGUES C.V., CERQUEIRA A.H., et al.
2011A&A...535A...2B viz 369     A     X         10 53 16 Will the starless cores in Chamaeleon I and III turn prestellar? BELLOCHE A., PARISE B., SCHULLER F., et al.
2011A&A...535A..16L 38           X         1 70 108 2MASS wide field extinction maps. IV. The Orion, Monoceros R2, Rosette, and Canis Major star forming regions. LOMBARDI M., ALVES J. and LADA C.J.
2011MNSSA..70..163S 24 0 Ophiuchus, the Herb Healer. STREICHER M.
2012ApJ...745...69K 16       D               2 136 429 A universal, local star formation law in galactic clouds, nearby galaxies, high-redshift disks, and starbursts. KRUMHOLZ M.R., DEKEL A. and McKEE C.F.
2012A&A...537L...9F 488 T K A     X         12 4 9 Chemical differentiation toward the Pipe Nebula starless cores. FRAU P., GIRART J.M. and BELTRAN M.T.
2012MNRAS.420..745C 101           X         1 1 124 TreeCol: a novel approach to estimating column densities in astrophysical simulations. CLARK P.C., GLOVER S.C.O. and KLESSEN R.S.
2012ApJ...747...22H 84           X         2 4 56 Feedback effects on low-mass star formation. HANSEN C.E., KLEIN R.I., McKEE C.F., et al.
2012A&A...538A.137M viz 39           X         1 41 28 A (sub)millimetre study of dense cores in Orion B9. MIETTINEN O., HARJU J., HAIKALA L.K., et al.
2012ApJ...747..149R 217     A     X         6 8 9 Barnard 59: no evidence for further fragmentation. ROMAN-ZUNIGA C.G., FRAU P., GIRART J.M., et al.
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