2MASS J05063495-0337158 , the SIMBAD biblio

2MASS J05063495-0337158 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST05:46:52


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in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2004A&A...416..677A 72 13 Multi-wavelength observations of the star forming region in L1616. ALCALA J.M., WACHTER S., COVINO E., et al.
2008ApJ...687.1303G 15       D               5 82 40 The star formation in the L1615/L1616 cometary cloud. GANDOLFI D., ALCALA J.M., LECCIA S., et al.
2014A&A...572A..84B 15       D   O           2 68 4 On the accretion properties of young stellar objects in the L1615/L1616 cometary cloud. BIAZZO K., ALCALA J.M., FRASCA A., et al.
2014ASPC..485..223B viz 15       D               1 465820 45 The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements BOURGES L., LAFRASSE S., MELLA G., et al.
2019AJ....158..122K viz 16       D               1 290057 150 Untangling the Galaxy. I. Local structure and star formation history of the Milky Way. KOUNKEL M. and COVEY K.
2019MNRAS.490.3158C viz 16       D               1 465839 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
2022ApJS..262....7H viz 17       D               1 134735 19 A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun. HE Z., WANG K., LUO Y., et al.
2023ApJS..265...12Q viz 17       D               1 58898 5 Hunting for Neighboring Open Clusters with Gaia DR3: 101 New Open Clusters within 500 pc. QIN S., ZHONG J., TANG T., et al.
2023A&A...674A..21M viz 17       D               1 11510 8 Gaia Data Release 3 Validating the classification of variable young stellar object candidates. MARTON G., ABRAHAM P., RIMOLDINI L., et al.
2024AJ....167..210V viz 18       D               1 7289 ~ The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. VACH S., ZHOU G., HUANG C.X., et al.

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