NAME Serpens South Cluster , the SIMBAD biblio

NAME Serpens South Cluster , the SIMBAD biblio (132 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:59:46

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Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2008ApJ...673L.151G 4 14 120 The Spitzer Gould belt survey of large nearby interstellar clouds: discovery of a dense embedded cluster in the Serpens-Aquila rift. GUTERMUTH R.A., BOURKE T.L., ALLEN L.E., et al.
2009ApJ...700.1609M 94       D       C       2 46 333 Filamentary structure of star-forming complexes. MYERS P.C.
2009ApJS..184...18G viz 38           X         1 2602 566 A Spitzer survey of young stellar clusters within one kiloparsec of the Sun: cluster core extraction and basic structural analysis. GUTERMUTH R.A., MEGEATH S.T., MYERS P.C., et al.
2010ApJ...716..634G 38           X         1 92 10 FLAMINGOS near infrared survey of the Serpens cloud main core. GORLOVA N., STEINHAUER A. and LADA E.
2010AJ....140..266W viz 76           X         2 259 58 The properties of X-ray luminous young stellar objects in the NGC 1333 and Serpens embedded clusters. WINSTON E., MEGEATH S.T., WOLK S.J., et al.
2010A&A...518L..85B 181     A     X C       4 9 121 The Herschel first look at protostars in the Aquila rift. BONTEMPS S., ANDRE P., KOENYVES V., et al.
2010ApJ...725.2485K viz 38           X         1 299 46 A Chandra observation of the obscured star-forming complex W40. KUHN M.A., GETMAN K.V., FEIGELSON E.D., et al.
2011ApJ...734...63S 1420 T K A S   X C       34 4 115 Near-infrared-imaging polarimetry toward Serpens south: revealing the importance of the magnetic field. SUGITANI K., NAKAMURA F., WATANABE M., et al.
2011ApJ...735...82M 154           X         4 15 24 Filamentary condensations in a young cluster. MYERS P.C.
2011ApJ...737...56N 1638 T   A     X C       41 8 44 Molecular outflows from the protocluster
Serpens South. 		NAKAMURA F., SUGITANI K., SHIMAJIRI Y., et al.
2011ApJ...740...36N 78           X         2 9 33 Clustered star formation in magnetic clouds: properties of dense cores formed in outflow-driven turbulence. NAKAMURA F. and LI Z.-Y.
2011A&A...535A..77M 2174     A S   X C       55 89 113 The formation of active protoclusters in the Aquila Rift: a millimeter continuum view. MAURY A.J., ANDRE P., MEN'SHCHIKOV A., et al.
2012ApJ...746...25N 78           X         2 16 52 Evidence for cloud-cloud collision and parsec-scale stellar feedback within the L1641-N region. NAKAMURA F., MIURA T., KITAMURA Y., et al.
2012ApJ...747...52D 45           X         1 13 163 Resolving the luminosity problem in low-mass star formation. DUNHAM M.M. and VOROBYOV E.I.
2012ApJ...752....9M 402       D     X         11 36 26 Mass and luminosity evolution of young stellar objects. MYERS P.C.
2012ApJ...754...10P 77           X         2 18 5 Far-ultraviolet observation of the Aquila Rift with FIMS/SPEAR. PARK S.-J., MIN K.-W., SEON K.-I., et al.
2012ApJ...754..104H 39           X         1 110 21 The Spitzer survey of interstellar clouds in the Gould Belt. V. Ophiuchus North observed with IRAC and MIPS. HATCHELL J., TEREBEY S., HUARD T., et al.
2012A&A...543A..51T 487 T   A     X         12 20 8 Molecular hydrogen jets and outflows in the
Serpens south filamentary cloud. 		TEIXEIRA G.D.C., KUMAR M.S.N., BACHILLER R., et al.
2012ApJ...756..105M 39           X         1 2 1 Gravitational stability of a cylindrical plasma with an azimuthal and an axial magnetic field. McLEMAN J.A., WANG C.H.-T. and BINGHAM R.
2013ApJ...762..128O viz 39           X         1 106 9 The physical structure of protoplanetary disks: the Serpens cluster compared with other regions. OLIVEIRA I., MERIN B., PONTOPPIDAN K.M., et al.
2013ApJ...764..140M 117           X         3 14 15 Origin of the dense core mass function in contracting filaments. MYERS P.C.
2013ApJ...766..115K 1632 T   A     X C       40 11 239 Filamentary accretion flows in the embedded
Serpens South protocluster. 		KIRK H., MYERS P.C., BOURKE T.L., et al.
2013A&A...553A..58L         O           127 13 Star-forming regions of the Aquila rift cloud complex. I. NH3 tracers of dense molecular cores. LEVSHAKOV S.A., HENKEL C., REIMERS D., et al.
2013ApJ...770..150H 50           X         1 3 67 Analytical theory for the initial mass function. III. Time dependence and star formation rate. HENNEBELLE P. and CHABRIER G.
2013ApJ...776...62H 79           X         2 7 19 Gravitational infall onto molecular filaments. II. Externally pressurized cylinders. HEITSCH F.
2013ApJ...778...34T 2753 T   A     X C       69 84 20 The dynamical state of the
Serpens South filamentary infrared dark cloud. 		TANAKA T., NAKAMURA F., AWAZU Y., et al.
2013MNRAS.436.1513F 3003 T   A D S   X C F     74 26 38 Abundant cyanopolyynes as a probe of infall in the Serpens south cluster-forming region. FRIESEN R.K., MEDEIROS L., SCHNEE S., et al.
2013ApJ...779..113M viz 39           X         1 367 28 The W40 region in the Gould belt: an embedded cluster and H II region at the junction of filaments. MALLICK K.K., KUMAR M.S.N., OJHA D.K., et al.
2014A&A...561A..83P viz 41           X         1 28 146 SDC13 infrared dark clouds: longitudinally collapsing filaments? PERETTO N., FULLER G.A., ANDRE Ph., et al.
2014MNRAS.438.1305H 79           X         2 7 11 Cluster formation in molecular clouds - I. Stellar populations, star formation rates and ionizing radiation. HOWARD C.S., PUDRITZ R.E. and HARRIS W.E.
2014ApJ...783...29D 39           X         1 73 94 Molecular outflows driven by low-mass protostars. I. Correcting for underestimates when measuring outflow masses and dynamical properties. DUNHAM M.M., ARCE H.G., MARDONES D., et al.
2014ApJ...783..115N 945     A D     X C       24 11 28 Confronting the outflow-regulated cluster formation model with observations. NAKAMURA F. and LI Z.-Y.
2014ApJ...784..116M 142     A     X         4 14 24 Lupus I observations from the 2010 flight of the balloon-borne large aperture submillimeter telescope for polarimetry. MATTHEWS T.G., ADE P.A.R., ANGILE F.E., et al.
2014ApJ...785...24T 42           X         1 9 56 Magnetohydrostatic equilibrium structure and mass of filamentary isothermal cloud threaded by lateral magnetic field. TOMISAKA K.
2014MNRAS.439.1996J 39           X         1 18 27 Gas kinematics and excitation in the filamentary IRDC G035.39-00.33. JIMENEZ-SERRA I., CASELLI P., FONTANI F., et al.
2014Sci...344..183K 2 18 102 Unfolding the laws of star formation: the density distribution of molecular coulds. KAINULAINEN J., FEDERRATH C. and HENNING T.
2014MNRAS.440.2860H 120           X         3 20 102 The dynamical properties of dense filaments in the infrared dark cloud G035.39-00.33. HENSHAW J.D., CASELLI P., FONTANI F., et al.
2014ApJ...790L..19F 47           X         1 5 80 CARMA large area star formation survey: observational analysis of filaments in the Serpens south molecular cloud. FERNANDEZ-LOPEZ M., ARCE H.G., LOONEY L., et al.
2014ApJ...791L..23N 619     A     X C       15 4 41 Cluster formation triggered by filament collisions in
Serpens South. 		NAKAMURA F., SUGITANI K., TANAKA T., et al.
2014ApJ...791..124G 51           X         1 6 145 Filaments in simulations of molecular cloud formation. GOMEZ G.C. and VAZQUEZ-SEMADENI E.
2014AJ....148...92R 1457     A D     X C       37 28 78 Young stellar object VARiability (YSOVAR): long timescale variations in the mid-infrared. REBULL L.M., CODY A.M., COVEY K.R., et al.
2014ApJ...797...76L 157           X         4 40 30 CARMA large area star formation survey: structure and kinematics of dense gas in Serpens main. LEE K.I., FERNANDEZ-LOPEZ M., STORM S., et al.
2015MNRAS.446.2118T 40           X         1 12 9 Polytropic models of filamentary interstellar clouds - II. Helical magnetic fields. TOCI C. and GALLI D.
2015ApJ...803...22P 3320 T K A S   X C       81 21 23 Assessing molecular outflows and turbulence in the protostellar cluster
Serpens South. 		PLUNKETT A.L., ARCE H.G., CORDER S.A., et al.
2015MNRAS.448.1551R viz 40           X         1 26 22 The JCMT Gould Belt Survey: evidence for radiative heating in Serpens MWC 297 and its influence on local star formation. RUMBLE D., HATCHELL J., GUTERMUTH R.A., et al.
2015ApJ...805....9O viz 2145     A D S   X C       53 164 12 The Gould's Belt Very Large Array survey. II. The Serpens region. ORTIZ-LEON G.N., LOINARD L., MIODUSZEWSKI A.J., et al.
2015A&A...577L...5A 373       D     X         10 14 27 Discovery of interstellar ketenyl (HCCO), a surprisingly abundant radical. AGUNDEZ M., CERNICHARO J. and GUELIN M.
2015ApJ...806..201S 278           X         7 18 5 Dense clumps and candidates for molecular outflows in W40. SHIMOIKURA T., DOBASHI K., NAKAMURA F., et al.
2015ApJS..219...21Z viz 79           X         2 59 8 A deep near-infrared survey toward the Aquila molecular cloud. I. Molecular hydrogen outflows. ZHANG M., FANG M., WANG H., et al.
2015ApJ...807...67M 47           X         1 3 46 The formation of filamentary bundles in turbulent molecular clouds. MOECKEL N. and BURKERT A.
2015ApJ...815...68M 423   K A S   X         10 4 21 Star cluster formation with stellar feedback and large-scale inflow. MATZNER C.D. and JUMPER P.H.
2015Natur.527...70P 466 T   A     X         11 6 64 Episodic molecular outflow in the very young protostellar cluster
Serpens South. 		PLUNKETT A.L., ARCE H.G., MARDONES D., et al.
2016AJ....151...42K 923           X C       22 30 6 Radio properties of young stellar objects in the core of the Serpens South Infrared Dark Cloud. KERN N.S., KEOWN J.A., TOBIN J.J., et al.
2016MNRAS.455.3640S 113           X         2 3 101 On the nature of star-forming filaments - II. Subfilaments and velocities. SMITH R.J., GLOVER S.C.O., KLESSEN R.S., et al.
2016MNRAS.456.4101L 41           X         1 13 18 The interstellar chemistry of H2C3O isomers. LOISON J.-C., AGUNDEZ M., MARCELINO N., et al.
2016ApJ...822...59S viz 40           X         1 4693 73 The Bolocam Galactic Plane Survey. XIV. Physical properties of massive starless and star-forming clumps. SVOBODA B.E., SHIRLEY Y.L., BATTERSBY C., et al.
2016ApJ...824...31L 40           X         1 27 21 Discovery of an extremely wide-angle bipolar outflow in AFGL 5142. LIU T., ZHANG Q., KIM K.-T., et al.
2016ApJ...824..136L 82   K       X         2 9 21 TMRT observations of carbon-chain molecules in

Serpens South 1a. 		LI J., SHEN Z.-Q., WANG J., et al.
2016AJ....152...36S viz 96       D       C       6 219 4 A catalog of low-mass star-forming cores observed with SHARC-II at 350 µm. SURESH A., DUNHAM M.M., ARCE H.G., et al.
2016A&A...592A..54A viz 4 17 80 Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArTeMiS. ANDRE P., REVERET V., KONYVES V., et al.
2016ApJ...831..189R 26 4 A multiwavelength characterization of proto-brown-dwarf candidates in Serpens. RIAZ B., VOROBYOV E., HARSONO D., et al.
2016A&A...594A..58O viz 40           X         1 8 3 The segregation of starless and protostellar clumps in the Hi-GAL l = 224° region. OLMI L., CUNNINGHAM M., ELIA D., et al.
2016ApJ...833..193R viz 80           X         2 1198 4 Young stellar populations in MYStIX star-forming regions: candidate protostars. ROMINE G., FEIGELSON E.D., GETMAN K.V., et al.
2016ApJ...833..204F 162           X         4 16 23 The fragmentation and stability of hierarchical structure in Serpens South. FRIESEN R.K., BOURKE T.L., DI FRANCESCO J., et al.
2017ApJ...835L..14G 42           X         1 12 19 L1188: a promising candidate for cloud-cloud collisions triggering the formation of low- and intermediate-mass stars. GONG Y., FANG M., MAO R., et al.
2017ApJ...836..133Z 81           X         2 23 4 Molecular outflows: explosive versus protostellar. ZAPATA L.A., SCHMID-BURGK J., RODRIGUEZ L.F., et al.
2017ApJS..229...28G viz 666       D     X         17 65 41 Star Formation in Nearby Clouds (SFiNCs): X-ray and infrared source catalogs and membership. GETMAN K.V., BROOS P.S., KUHN M.A., et al.
2017MNRAS.466.4633A 41           X         1 11 1 On the impact of the magnitude of interstellar pressure on physical properties of molecular cloud. ANATHPINDIKA S., BURKERT A. and KUIPER R.
2017ApJ...848...51D 41           X         1 16 1 Embedded filaments in IRAS 05463+2652: early stage of fragmentation and star formation activities. DEWANGAN L.K., DEVARAJ R., BAUG T., et al.
2017ApJ...849...43H 625       D S   X         15 133 49 How do stars gain their mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star-forming Regions. HERCZEG G.J., JOHNSTONE D., MAIRS S., et al.
2018ApJ...852...12Y 42           X         1 35 54 High-mass star formation through filamentary collapse and clump-fed accretion in G22. YUAN J., LI J.-Z., WU Y., et al.
2018AJ....155...99W viz 1836 T   A S   X C       42 1542 7 YSOVAR: mid-infrared variability among YSOs in the star formation region
Serpens South. 		WOLK S.J., GUNTHER H.M., POPPENHAEGER K., et al.
2018MNRAS.476.1213G viz 41           X         1 32 14 Intracluster age gradients in numerous young stellar clusters. GETMAN K.V., FEIGELSON E.D., KUHN M.A., et al.
2018AJ....155..241W viz 3194 T   A S   X C       75 324 5 Chandra detection of an evolved population of young stars in
Serpens South. 		WINSTON E., WOLK S.J., GUTERMUTH R., et al.
2018ApJ...861..145C 165           X         4 101 84 A near-infrared spectroscopic survey of FU Orionis objects. CONNELLEY M.S. and REIPURTH B.
2018A&A...615A...9P viz 2330 T   A     X         56 98 38 Distribution of

Serpens South protostars revealed with ALMA. 		PLUNKETT A.L., FERNANDEZ-LOPEZ M., ARCE H.G., et al.
2018ApJ...864..172H 247           X         6 25 ~ Variability and jet activity in the YSO MHO 3252 Y3 in Serpens South. HODAPP K.W. and CHINI R.
2018ApJ...869L..33O 725     A     X         18 46 88 Gaia-DR2 confirms VLBA parallaxes in Ophiuchus, Serpens, and Aquila. ORTIZ-LEON G.N., LOINARD L., DZIB S.A., et al.
2019ApJ...874..172K viz 1404     A     X         34 6 ~ H2CO and H110α observations toward the Aquila Molecular Cloud. KOMESH T., ESIMBEK J., BAAN W., et al.
2019ApJ...875...24C 47           X         1 10 56 Filamentary accretion flows in the infrared dark cloud G14.225-0.506 revealed by ALMA. CHEN H.-R.V., ZHANG Q., WRIGHT M.C.H., et al.
2019ApJ...878..111H viz 42           X         1 3863 48 An initial overview of the extent and structure of recent star formation within the Serpens Molecular Cloud using Gaia Data Release 2. HERCZEG G.J., KUHN M.A., ZHOU X., et al.
2019A&A...626A..79P viz 42           X         1 1887 ~ Do star clusters form in a completely mass-segregated way? PAVLIK V., KROUPA P. and SUBR L.
2019MNRAS.487..887R 334           X C F     6 5 ~ Spatial statistics in star-forming regions: testing the limits of randomness. RETTER B., HATCHELL J. and NAYLOR T.
2019MNRAS.488..495W 42           X         1 52 ~ Carbon-chain molecules in molecular outflows and Lupus I region - new producing region and new forming mechanism. WU Y., LIU X., CHEN X., et al.
2019ApJ...883....1Z 44           X         1 11 28 An episodic wide-angle outflow in HH 46/47. ZHANG Y., ARCE H.G., MARDONES D., et al.
2020MNRAS.491..440W 48           X         1 8 43 The possible role of stellar mergers for the formation of multiple stellar populations in globular clusters. WANG L., KROUPA P., TAKAHASHI K., et al.
2020ApJ...892..122J 43           X         1 14 ~ A novel survey for young substellar objects with the W-band filter. II. The coolest and lowest mass members of the Serpens-South star-forming region. JOSE J., BILLER B.A., ALBERT L., et al.
2020A&A...636A..38N viz 44           X         1 17 26 Episodic accretion constrained by a rich cluster of outflows. NONY T., MOTTE F., LOUVET F., et al.
2020MNRAS.495.3614C viz 868       D     X C       20 75 19 The relationship between mid-infrared and sub-millimetre variability of deeply embedded protostars. CONTRERAS PENA C., JOHNSTONE D., BAEK G., et al.
2020A&A...638A.155P 43           X         1 2 ~ Primordial mass segregation of star clusters with primordial binaries. PAVLIK V.
2020A&A...639A..80S 469           X C F     9 12 20 Diffuse γ-ray emission toward the massive star-forming region, W40. SUN X.-N., YANG R.-Z., LIANG Y.-F., et al.
2020ApJ...900...82P 140           X C       2 6 77 The origin of massive stars: the inertial-inflow model. PADOAN P., PAN L., JUVELA M., et al.
2020MNRAS.497.4517S 43           X         1 6 ~ The highly variable time evolution of star-forming cores identified with dendrograms. SMULLEN R.A., KRATTER K.M., OFFNER S.S.R., et al.
2020A&A...642A..76Z viz 43           X         1 68 19 Fragmentation of star-forming filaments in the X-shaped nebula of the California molecular cloud. ZHANG G.-Y., ANDRE P., MEN'SHCHIKOV A., et al.
2020A&A...642A..87K viz 44           X         1 37 59 Unifying low- and high-mass star formation through density-amplified hubs of filaments. The highest mass stars (>100 M☉) form only in hubs. KUMAR M.S.N., PALMEIRIM P., ARZOUMANIAN D., et al.
2019PASJ...71S...3N 209           X C       4 33 28 Nobeyama 45 m mapping observations toward the nearby molecular clouds Orion A, Aquila Rift, and M17: Project overview. NAKAMURA F., ISHII S., DOBASHI K., et al.
2019PASJ...71S...4S 3327 T   A S   X C       77 8 ~ Cluster formation in the W 40 and
Serpens South complex triggered by the expanding H II region. 		SHIMOIKURA T., DOBASHI K., NAKAMURA F., et al.
2020A&A...643A.178T 3235     A D     X C       76 32 ~ Ammonia observations towards the Aquila Rift cloud complex. TURSUN K., ESIMBEK J., HENKEL C., et al.
2020ApJS..251...26L viz 43           X         1 11 ~ CO outflow candidates toward the W3/4/5 Complex. II. Feedback from candidate outflows. LI Y., XU Y., SUN Y., et al.
2020A&A...644A.128S 43           X         1 43 ~ VLA ammonia observations of L1287. Analysis of the Guitar core and two filaments. SEPULVEDA I., ESTALELLA R., ANGLADA G., et al.
2021A&A...645A..94N viz 44           X         1 277 20 Mass segregation and sequential star formation in NGC 2264 revealed by Herschel. NONY T., ROBITAILLE J.-F., MOTTE F., et al.
2021ApJ...908...70H 131           X         3 17 ~ DR 21 South Filament: a parsec-sized dense gas accretion flow onto the DR 21 massive young cluster. HU B., QIU K., CAO Y., et al.
2019PASJ...71S...5K 2257 T         X C       52 8 ~ Magnetic field structure in
Serpens South. 		KUSUNE T., NAKAMURA F., SUGITANI K., et al.
2019PASJ...71S...6S 2257 T         X C       52 61 ~ A survey of molecular cores in M 17 SWex. SHIMOIKURA T., DOBASHI K., HIROSE A., et al.
2019PASJ...71S...7S 2257 T         X C       52 20 ~ Near-infrared imaging polarimetry toward M17SWex. SUGITANI K., NAKAMURA F., SHIMOIKURA T., et al.
2019PASJ...71S...8T 42           X         1 45 ~ Nobeyama 45 m mapping observations toward Orion A. I. Molecular outflows. TANABE Y., NAKAMURA F., TSUKAGOSHI T., et al.
2019PASJ...71S..10N 42           X         1 21 ~ Nobeyama 45 m mapping observations towardOrion A. III. Multi-line observations toward an outflow-shocked region, Orion Molecular Cloud 2 FIR 4. NAKAMURA F., OYAMADA S., OKUMURA S., et al.
2021A&A...649A.113B viz 87           X         2 46 14 Fragmentation and kinematics in high-mass star formation. CORE-extension targeting two very young high-mass star-forming regions. BEUTHER H., GIESER C., SURI S., et al.
2021A&A...650A.157G viz 17       D               1 81 9 Dispersal timescale of protoplanetary disks in the low-metallicity young cluster Dolidze 25. GUARCELLO M.G., BIAZZO K., DRAKE J.J., et al.
2021AJ....162...68O 810 T   A     X C       17 31 2 Discovery of 22 GHz water masers in the
Serpens South region. 		ORTIZ-LEON G.N., PLUNKETT A.L., LOINARD L., et al.
2021MNRAS.507.1904R 2699     A D     X C F     61 26 3 Spatial statistics in star-forming regions: is star formation driven by column density alone? RETTER B., HATCHELL J. and NAYLOR T.
2021ApJ...920..119L 627       D S   X         14 55 18 The JCMT Transient Survey: four-year summary of monitoring the submillimeter variability of protostars. LEE Y.-H., JOHNSTONE D., LEE J.-E., et al.
2022ApJ...924L..23Z 46           X         1 11 14 The rate, amplitude, and duration of outbursts from Class 0 protostars in Orion. ZAKRI W., MEGEATH S.T., FISCHER W.J., et al.
2022ApJ...924...81P 45           X         1 13 1 Rebounding cores to build star cluster multiple populations. PARMENTIER G. and PASQUALI A.
2022PASJ...74...24K 45           X         1 50 3 Nobeyama 45 m Local Spur CO survey. I. Giant molecular filaments and cluster formation in the Vulpecula OB association. KOHNO M., NISHIMURA A., FUJITA S., et al.
2022ApJ...928...76S 45           X         1 6 ~ Cluster Formation in GGD 12-15: Infall Motion with Rotation of the Natal Clump. SHIMOIKURA T., DOBASHI K., HIRANO N., et al.
2022MNRAS.513.1275A 45           X         1 15 ~ Core formation via filament fragmentation and the impact of ambient pressure on it. ANATHPINDIKA S.V. and DI FRANCESCO J.
2022A&A...662A.104D 45           X         1 12 2 SOLIS. XVI. Mass ejection and time variability in protostellar outflows: Cep E. DE SCHUTZER A.A., RIVERA-ORTIZ P.R., LEFLOCH B., et al.
2022ApJ...933...77Z 296     A     X         7 30 3 The Ages of Optically Bright Subclusters in the Serpens Star-forming Region. ZHOU X., HERCZEG G.J., LIU Y., et al.
2022A&A...663L...5C 45           X         1 7 4 Discovery of five cyano derivatives of propene with the QUIJOTE line survey. CERNICHARO J., FUENTETAJA R., CABEZAS C., et al.
2022MNRAS.516.1983S 45           X         1 14 5 ATOMS: ALMA three-millimeter observations of massive star-forming regions - XII: Fragmentation and multiscale gas kinematics in protoclusters G12.42+0.50 and G19.88-0.53. SAHA A., TEJ A., LIU H.-L., et al.
2022ApJ...937....6J 108       D     X         3 20 2 The JCMT Transient Survey: Single-epoch Transients and Variability of Faint Sources. JOHNSTONE D., LALCHAND B., MAIRS S., et al.
2022MNRAS.516.5244S 90             C       1 8 3 Deep near-infrared survey towards the W40 and Serpens South region in the Aquila Rift: A comprehensive catalogue of young stellar objects. SUN J., GUTERMUTH R.A., WANG H., et al.
2022MNRAS.516.5258S 179           X C       3 7 1 Hierarchical structure of YSO clusters in the W40 and Serpens South region: group extraction and comparison with fractal clusters. SUN J., GUTERMUTH R.A., WANG H., et al.
2022ApJ...939L..10P 18       D               1 68 10 Most Planets Might Have More than 5 Myr of Time to Form. PFALZNER S., DEHGHANI S. and MICHEL A.
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