NAME the Pipe Nebula , the SIMBAD biblio

NAME the Pipe Nebula , the SIMBAD biblio (370 results) C.D.S. - SIMBAD4 rel 1.8 - 2022.06.30CEST15:15:02


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Title First 3 Authors
1995MNSSA..54...72. 127 0 The nomenclature of deep-sky objects. :Anonymous
1999PASJ...51..871O 73 T                   29 58 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 75 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 59 High-mass cloud cores in the η Carinae giant molecular cloud. YONEKURA Y., ASAYAMA S., KIMURA K., et al.
2006A&A...453..635M viz 8 15 251 Modelling the Galactic interstellar extinction distribution in three dimensions. MARSHALL D.J., ROBIN A.C., REYLE C., et al.
2006A&A...454..781L 120 T K                 9 135 2MASS wide field extinction maps. I.
The Pipe nebula.
LOMBARDI M., ALVES J. and LADA C.J.
2007ApJ...655..364B 37 42 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 21 6 259 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 43           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 1842 T K A S   X C       46 103 24 An accurate determination of the distance to the
Pipe nebula.
ALVES F.O. and FRANCO G.A.P.
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 48 66 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 34 Massive clumps in the NGC 6334 star-forming region. MUNOZ D.J., MARDONES D., GARAY G., et al.
2007MNRAS.381L..40D 47           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 9 30 571 Cold dark clouds : the initial conditions for star formation. BERGIN E.A. and TAFALLA M.
2007ApJ...671.1820M 744 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 486 T   A     X C       11 11 131 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 1359 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 55           X         1 3 105 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 40           X         1 8 40 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 3 15 117 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 195           X         5 5 40 On the evolution of the dense core mass function. SWIFT J.J. and WILLIAMS J.P.
2008ApJ...681..365E 115           X         3 20 64 On the constancy of the characteristic mass of young stars. ELMEGREEN B.G., KLESSEN R.S. and WILSON C.D.
2008A&A...486L..13A 943 T K A S   X C       22 5 51 Optical polarimetry toward the
Pipe nebula: revealing the importance of the magnetic field.
ALVES F.O., FRANCO G.A.P. and GIRART J.M.
2008ApJ...682.1095B 153           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 229           X         6 220 169 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 458           X C       11 33 64 2MASS wide field extinction maps. II. The Ophiuchus and the Lupus cloud complexes. LOMBARDI M., LADA C.J. and ALVES J.
2008MNRAS.390..807C 343     A D     X C F     8 12 3 The directional analysis of star clusters. CARTWRIGHT A. and WHITWORTH A.P.
2008ApJ...687..340M 114           X         3 15 28 Protostar mass due to infall and dispersal. MYERS P.C.
2008ApJ...687..354N 484     A S   X C       11 13 84 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 77           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 391           X C       9 3 46 Nicest, a near-infrared color excess method tailored to small-scale structures. LOMBARDI M.
2009MNRAS.392..341C 207       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 99 The "True" column density distribution in star-forming molecular clouds. GOODMAN A.A., PINEDA J.E. and SCHNEE S.L.
2009NewA...14..221B 78           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 115           X         3 22 20 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 968 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 195           X C F     3 2 14 The inevitable future of the starless core Barnard 68. BURKERT A. and ALVES J.
2009ApJ...696..298F viz 117           X         3 9 41 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 1067     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 154           X         4 48 47 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 41 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 65 The structure of molecular clouds - I. All-sky near-infrared extinction maps. ROWLES J. and FROEBRICH D.
2009MNRAS.396..830S 42           X         1 6 48 Fragmentation in molecular clouds and its connection to the IMF. SMITH R.J., CLARK P.C. and BONNELL I.A.
2009ApJ...699..585H 361       D     X         10 147 28 A search for carbon-chain-rich cores in dark clouds. HIROTA T., OHISHI M. and YAMAMOTO S.
2009ApJ...699..742R viz 1582 T   A D S   X C F     38 3 51 Dense cores in the
Pipe Nebula: an improved core mass function.
RATHBORNE J.M., LADA C.J., MUENCH A.A., et al.
2008BaltA..17..253S 37 22 2MASS two-color interstellar reddening lines in the inner galaxy. STRAIZYS V. and LAUGALYS V.
2009ApJ...700.1541R 77           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 116           X C       2 46 111 Filamentary structure of star-forming complexes. MYERS P.C.
2009ApJ...702..352L 156           X C       3 13 56 The structure of a low-metallicity giant molecular cloud complex. LEROY A.K., BOLATTO A., BOT C., et al.
2009ApJ...702.1428H 49           X         1 4 89 Analytical theory for the initial mass function. II. Properties of the flow. HENNEBELLE P. and CHABRIER G.
2009A&A...503..859B viz 215     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 77           X         2 62 48 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 562 T   A     X         14 8 21 High resolution near-infrared survey of the
Pipe Nebula. I. A deep infrared extinction map of Barnard 59.
ROMAN-ZUNIGA C.G., LADA C.J. and ALVES J.F.
2009ApJ...704..292F 1406 T   A S   X C       34 48 32 A Spitzer census of star formation activity in the
Pipe Nebula.
FORBRICH J., LADA C.J., MUENCH A.A., et al.
2009ApJ...704..531K viz 15       D     X         1 181 65 The coevality of young binary systems. KRAUS A.L. and HILLENBRAND L.A.
2009ApJ...704.1735H 412 T   A S   X         9 4 43 Gravitational collapse and filament formation: comparison with the Pipe Nebula. HEITSCH F., BALLESTEROS-PAREDES J. and HARTMANN L.
2009ApJ...707...89G viz 40           X         1 8 33 Mid-infrared extinction and its variation with galactic longitude. GAO J., JIANG B.W. and LI A.
2009ApJ...706.1341M 79           X         2 5 25 On the distribution of protostar masses. MYERS P.C.
2009ApJ...707.1824N viz 115           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 44           X         1 10 118 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 95       D   O X         3 25 165 Probing the evolution of molecular cloud structure. From quiescence to birth. KAINULAINEN J., BEUTHER H., HENNING T., et al.
2010A&A...509A..44M 39           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 43           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 46 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 155           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 39           X         1 60 87 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 53         O X         1 15 431 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 40           X         1 10 34 The protostellar mass function. McKEE C.F. and OFFNER S.S.R.
2010ApJ...716..433K 969     A D     X C       25 16 81 The mass-size relation from clouds to cores. II. Solar neighborhood clouds. KAUFFMANN J., PILLAI T., SHETTY R., et al.
2010ApJ...716..893P viz 77           X         2 42 25 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 39           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 116           X         3 24 44 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 46 Collision between dissimilar clouds: stability of the bow-shock, and the formation of pre-stellar cores. ANATHPINDIKA S.V.
2010MNRAS.406..505S 39           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 1300 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 39           X         1 5 9 The evolution of cloud cores and the formation of stars. BRODERICK A.E. and KETO E.
2010ApJ...721.1206C 77           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 39           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 39           X         1 41 28 Have protoplanetary discs formed planets{quest}. GREAVES J.S. and RICE W.K.M.
2010ApJ...722..971C 526     A     X C       13 78 58 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 85           X         2 7 124 How many infrared dark clouds can form massive stars and clusters? KAUFFMANN J. and PILLAI T.
2010ApJ...723..146F 2191 T K A     X C       55 24 58 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 171       D       C F     4 27 70 Larson's third law and the universality of molecular cloud structure. LOMBARDI M., ALVES J. and LADA C.J.
2010ApJ...723.1065O 39           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 1532 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 203           X         5 19 386 On the star formation rates in molecular clouds. LADA C.J., LOMBARDI M. and ALVES J.F.
2010A&A...520A..17K 42           X         1 25 178 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 31 Do lognormal column-density distributions in molecular clouds imply supersonic turbulence ? TASSIS K., CHRISTIE D.A., URBAN A., et al.
2010ApJ...725.1327S 271           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 1378 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 116           X         3 35 12 Physical properties of dense cores in Orion B9. MIETTINEN O., HARJU J., HAIKALA L.K., et al.
2011ApJ...726...46N 156           X         4 39 27 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 55       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 47           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 39           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 117           X         3 102 58 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         2 144 191 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 40           X         1 15 42 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 156           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 118           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 80 The link between molecular cloud structure and turbulence. SCHNEIDER N., BONTEMPS S., SIMON R., et al.
2011NewAR..55...23V 16       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 212       D     X         6 26 69 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 60 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 39           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 39           X         1 233 49 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 273           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 39           X         1 15 24 Filamentary condensations in a young cluster. MYERS P.C.
2011ApJ...736..149G 39           X         1 35 22 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 39           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 39           X         1 16 3 Prestellar cores in the Coalsack. SAUL M., CUNNINGHAM M., RATHBORNE J., et al.
2011ApJ...739...25M 42           X         1 15 115 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 39           X         1 489 46 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 51           X         1 2 49 Does external pressure explain recent results for molecular clouds? FIELD G.B., BLACKMAN E.G. and KETO E.R.
2011MNRAS.416..783P 40           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 195           X         5 171 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 374     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 39           X         1 70 74 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 17       D               2 136 291 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 497 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 74           X         1 1 71 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 86           X         2 4 56 Feedback effects on low-mass star formation. HANSEN C.E., KLEIN R.I., McKEE C.F., et al.
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