2MASS J18294878+0113422 , the SIMBAD biblio

2MASS J18294878+0113422 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.07.31CEST21:23:43


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Title First 3 Authors
2015ApJS..220...11D viz 16       D               1 2988 78 Young stellar objects in the Gould belt. DUNHAM M.M., ALLEN L.E., EVANS II N.J., 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.
2009ApJS..181..321E viz 15       D               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.
2009ApJS..184...18G viz 15       D               2 2602 235 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.
2007ApJ...663.1149H viz 15       D               580 131 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 80 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.
2004A&A...421..623K viz 167 67 The young stellar population in the Serpens Cloud Core: An ISOCAM survey. KAAS A.A., OLOFSSON G., BONTEMPS S., et al.
2004A&A...425..927K viz 26 4 Substellar objects in star formation regions: A deep near infrared study in the Serpens cloud. KLOTZ A., CAUX E., MONIN J.-L., et al.
1999AJ....118..558K 106 44 K-band variability as a method to select young stellar object candidates. KAAS A.A.
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.
1992A&A...262..468E 163 108 Near-infrared images of the Serpens cloud core: the stellar cluster. EIROA C. and CASALI M.M.

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2021.07.31-21:23:43

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