2MASS J18312765-0205096 , the SIMBAD biblio

2MASS J18312765-0205096 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST10:08:20


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Title First 3 Authors
1985ApJ...291..571S 19 23 Infrared sources and excitation of the W 40 complex. SMITH J., BENTLEY A., CASTELAZ M., et al.
2010AJ....140..968R viz 15       D               2 24 13 A cluster of compact radio sources in W40. RODRIGUEZ L.F., RODNEY S.A. and REIPURTH B.
2010ApJ...725.2485K viz 15       D               1 299 46 A Chandra observation of the obscured star-forming complex W40. KUHN M.A., GETMAN K.V., FEIGELSON E.D., et al.
2012AJ....144..116S 92       D     X         3 22 15 Spectral classification of the brightest objects in the galactic star-forming region W40. SHUPING R.Y., VACCA W.D., KASSIS M., et al.
2013ApJ...779..113M viz 15       D               2 367 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.
2015ApJ...805....9O viz 16       D               2 164 12 The Gould's Belt Very Large Array survey. II. The Serpens region. ORTIZ-LEON G.N., LOINARD L., MIODUSZEWSKI A.J., et al.
2016MNRAS.460.4150R viz 16       D               4 283 12 The JCMT Gould Belt Survey: evidence for radiative heating and contamination in the W40 complex. RUMBLE D., HATCHELL J., PATTLE K., et al.
2017ApJ...834..143O 17       D               1 50 107 The Gould's Belt Distances Survey (GOBELINS). III. The distance to the Serpens/Aquila molecular complex. ORTIZ-LEON G.N., DZIB S.A., KOUNKEL M.A., et al.
2018ApJ...869L..33O 17       D               2 46 88 Gaia-DR2 confirms VLBA parallaxes in Ophiuchus, Serpens, and Aquila. ORTIZ-LEON G.N., LOINARD L., DZIB S.A., et al.
2021ApJ...916...32G viz 17       D               1 1084 20 X-ray superflares from pre-main-sequence stars: flare energetics and frequency. GETMAN K.V. and FEIGELSON E.D.
2021ApJ...920..154G 17       D               1 67 11 X-ray superflares from pre-main-sequence stars: flare modeling. GETMAN K.V., FEIGELSON E.D. and GARMIRE G.P.

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