V* V2755 Ori , the SIMBAD biblio

V* V2755 Ori , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:16:55


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Title First 3 Authors
1996A&AS..119....7A 164 117 New weak-line T Tauri stars in Orion from the ROSAT all-sky survey. ALCALA J.M., TERRANEGRA L., WICHMANN R., et al.
2000A&A...353..186A 123 54 High-resolution spectroscopy of ROSAT low-mass pre-main sequence stars in Orion. ALCALA J.M., COVINO E., TORRES G., 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.
2007A&A...463.1081M         O           49 15 Rotational periods of solar-mass young stars in Orion. MARILLI E., FRASCA A., COVINO E., et al.
2010ApJ...723.1542X viz 15       D               1 128 12 Lithium abundances from optical high-resolution spectroscopy of weak-line T Tauri stars. XING L.F.
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.
2005yCat.3244....0G viz 15       D               2 26640 61 Catalog of Stellar Rotational Velocities GLEBOCKI R. and GNACINSKI P.
2018A&A...620A.172Z viz 16       D               1 127610 99 3D mapping of young stars in the solar neighbourhood with Gaia DR2. ZARI E., HASHEMI H., BROWN A.G.A., 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.
2022ApJ...931..156P viz 17       D               1 22106 16 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR 3. II. Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures. PANG X., TANG S.-Y., LI Y., 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.
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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