2MASS J18295655+0112596 , the SIMBAD biblio

2MASS J18295655+0112596 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST23:00:25


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Title First 3 Authors
1988A&A...201..299G 20 38 Observational evidence for the influence of the magnetic field on star formation in the Serpens molecular cloud. GOMEZ DE CASTRO A.I., EIROA C. and LENZEN R.
1989A&A...223L..17E 14 39 The Serpens sources SVS 4 and FIRS 1 : new results from infrared images. EIROA C. and CASALI M.M.
1992A&A...262..468E 163 117 Near-infrared images of the Serpens cloud core: the stellar cluster. EIROA C. and CASALI M.M.
1997AJ....113.1057S 44 24 Infrared polarimetry of star-forming regions: the Serpens cloud core. SOGAWA H., TAMURA M., GATLEY I., et al.
1998A&A...330..990G viz 166 40 Deep optical and near infrared imaging photometry of the Serpens cloud core. GIOVANNETTI P., CAUX E., NADEAU D., et al.
2003A&A...401..613A viz         O           61 36 ISOCAM-CVF spectroscopy of the circumstellar environment of young stellar objects. ALEXANDER R.D., CASALI M.M., ANDRE P., et al.
2004A&A...421..623K viz 166 77 The young stellar population in the Serpens Cloud Core: An ISOCAM survey. KAAS A.A., OLOFSSON G., BONTEMPS S., et al.
2004A&A...426..925P 2         O           17 134 Mapping ices in protostellar environments on 1000 AU scales. Methanol-rich ice in the envelope of Serpens SMM 4. PONTOPPIDAN K.M., VAN DISHOECK E.F. and DARTOIS E.
2005AJ....130..643E 29 21 Very large array 3.5 cm continuum sources in the Serpens cloud core. EIROA C., TORRELLES J.M., CURIEL S., et al.
2006AN....327...14E 15 3 Brown dwarf candidates in the Serpens cloud core. EIROA C., DJUKVIP A.A. and CASALI M.M.
2007A&A...463..275G viz 15       D               121 32 The onset of X-ray emission in young stellar objects. A Chandra observation of the Serpens star-forming region. GIARDINO G., FAVATA F., MICELA G., et al.
2007ApJ...663.1149H viz 15       D               580 171 The Spitzer c2d survey of large, nearby, interstellar clouds. IX. The Serpens YSO population as observed with IRAC and MIPS. HARVEY P., MERIN B., HUARD T.L., et al.
2007ApJ...669..493W viz 15       D               1 154 101 A combined Spitzer and Chandra survey of young stellar objects in the Serpens cloud core. WINSTON E., MEGEATH S.T., WOLK S.J., et al.
2009A&A...495..837G 15       D   O           4 89 21 Lack of PAH emission toward low-mass embedded young stellar objects. GEERS V.C., VAN DISHOECK E.F., PONTOPPIDAN K.M., et al.
2009ApJS..181..321E viz 15       D               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.
2009ApJS..184...18G viz 15       D               2 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..299S 244       D     X C       6 49 27 Near-infrared imaging polarimetry of the Serpens cloud core: magnetic field structure, outflows, and inflows in a cluster forming clump. SUGITANI K., NAKAMURA F., TAMURA M., et al.
2013ApJS..205....5H viz 16       D               1 1329 12 Populations of young stellar objects in nearby molecular clouds. HSIEH T.-H. and LAI S.-P.
2014A&A...572A..62A 16       D               5 158 21 POISSON project. III. Investigating the evolution of the mass accretion rate. ANTONIUCCI S., GARCIA LOPEZ R., NISINI B., et al.
2015A&A...573A.100F viz 16       D               1 335 8 The WFCAM multiwavelength Variable Star Catalog. FERREIRA LOPES C.E., DEKANY I., CATELAN M., et al.
2015ApJS..220...11D viz 16       D               1 2988 232 Young stellar objects in the Gould belt. DUNHAM M.M., ALLEN L.E., EVANS II N.J., et al.
2020A&A...643A..48P viz 102       D         F     6 21 16 Linking ice and gas in the Serpens low-mass star-forming region. PEROTTI G., ROCHA W.R.M., JORGENSEN J.K., et al.
2021ApJ...920..132P viz 17       D               1 5441 33 Quantifying variability of young stellar objects in the mid-infrared over 6 years with the Near-Earth Object Wide-field Infrared Survey Explorer. PARK W., LEE J.-E., CONTRERAS PENA C., et al.

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