V* V604 Aur , the SIMBAD biblio

V* V604 Aur , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST15:23:32


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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.
2007A&A...467..785N viz 434 127 New periodic variable stars coincident with ROSAT sources discovered using SuperWASP. NORTON A.J., WHEATLEY P.J., WEST R.G., et al.
2009ApJS..184..138H viz 15       D               2 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.
2011IBVS.5969....1K viz 15       D               1 2041 27 The 80th name-list of variable stars. Part I - RA 0h to 6h. KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al.
2011AJ....142..138L viz 15       D               1 8898 232 An all-sky catalog of bright M dwarfs. LEPINE S. and GAIDOS E.
2013MNRAS.435.2161F viz 15       D               1 8411 18 A catalogue of bright (K < 9) M dwarfs. FRITH J., PINFIELD D.J., JONES H.R.A., et al.
2019ApJ...877...60B viz 16       D               1 658 26 The elusive majority of young moving groups. I. Young binaries and lithium-rich stars in the solar neighborhood. BOWLER B.P., HINKLEY S., ZIEGLER C., 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.
2021A&A...649A...6G viz 17       D               1 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2023AJ....165..267H viz 17       D               1 64663 1 Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., 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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