2MASS J06322611+1019184 , the SIMBAD biblio

2MASS J06322611+1019184 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST20:19:13


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Title First 3 Authors
2010AJ....140.1214C viz 15       D               1 151 114 A near-infrared spectroscopic survey of class I protostars. CONNELLEY M.S. and GREENE T.P.
2011AJ....141...40C 212     A     X         6 42 47 PTF10nvg: an outbursting class I protostar in the Pelican/North american nebula. COVEY K.R., HILLENBRAND L.A., MILLER A.A., et al.
2018ApJ...861..145C 257       D     X         7 101 84 A near-infrared spectroscopic survey of FU Orionis objects. CONNELLEY M.S. and REIPURTH B.
2019MNRAS.486.4590C viz 16       D               1 154 35 Determining the recurrence time-scale of long-lasting YSO outbursts. CONTRERAS PENA C., NAYLOR T. and MORRELL S.
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.
2020MNRAS.492..294G 41           X         1 29 ~ Short- and long-term near-infrared spectroscopic variability of eruptive protostars from VVV. GUO Z., LUCAS P.W., CONTRERAS PENA C., et al.
2021MNRAS.500.2440M 42           X         1 48 ~ New Herbig-Haro objects and outflows in the Mon R1 association. MOVSESSIAN T.A., MAGAKIAN T.Y. and DODONOV S.N.
2022MNRAS.510.2139M 443       D S   X   F     9 21 ~ Near-infrared detection of H2 flows in the core of the Mon R1 association. MAGAKIAN T.Y., TATARNIKOV A.M., MOVSESSIAN T.A., 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.
2023A&A...672A.158S 17       D               4 62 1 The Effelsberg survey of FU Orionis and EX Lupi objects I. Host environments of FUors and EXors traced by NH3. SZABO Z.M., GONG Y., MENTEN K.M., et al.
2023A&A...674A.202S 17       D               1 67 ~ The Effelsberg survey of FU Orionis and EX Lupi objects II. H2O maser observations. SZABO Z.M., GONG Y., YANG W., et al.

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