2MASS J03164389+1923041 , the SIMBAD biblio

2MASS J03164389+1923041 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST15:16:45


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Title First 3 Authors
1998A&AS..132..173L viz 177 42 Newly discovered candidate weak-line T Tauri stars in the surrounding area of the Taurus-Auriga region. LI J.Z. and HU J.Y.
2003A&A...406..535Z viz 15       D               1 10257 80 The Hamburg/RASS Catalogue of optical identifications. Northern high-galactic latitude ROSAT Bright Source Catalogue X-ray sources. ZICKGRAF F.-J., ENGELS D., HAGEN H.-J., et al.
2005A&A...438..769D viz 1380 87 Pre-main sequence star Proper Motion Catalogue. DUCOURANT C., TEIXEIRA R., PERIE J.-P., et al.
2006PASP..118.1690M viz 15       D               332 82 The formation and evolution of planetary systems: placing our solar system in context with Spitzer. MEYER M.R., HILLENBRAND L.A., BACKMAN D., et al.
2008ApJS..179..423C 15       D               3 334 51 The formation and evolution of planetary systems: description of the spitzer legacy science database. CARPENTER J.M., BOUWMAN J., SILVERSTONE M.D., et al.
2009ApJS..181..197C 15       D               1 324 164 Formation and evolution of planetary systems: properties of debris dust around solar-type stars. CARPENTER J.M., BOUWMAN J., MAMAJEK E.E., et al.
2009ApJS..184..138H viz 15       D               1 20623 68 XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. HAAKONSEN C.B. and RUTLEDGE R.E.
2010MNRAS.408..475H viz 15       D               2 1926 134 A large sample of photometric rotation periods for FGK Pleiades stars. HARTMAN J.D., BAKOS G.A., KOVACS G., et al.
2016A&A...593L..18C viz 16       D               1 361 1 Pseudomagnitude distances: Application to the Pleiades cluster. CHELLI A. and DUVERT G.
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.

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