HD 26929 , the SIMBAD biblio

HD 26929 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST16:54:59


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Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
1967PASP...79...72K 75 0 Identifications of comparison stars for RR Lyrae variables. KIM J. and STURCH C.
1989ApJS...69..593L 56 77 The luminosity scale of RR Lyrae stars with the Baade-Wesselink method. I. Photometry and radial velocities. LIU T.-X. and JANES K.A.
1991IBVS.3554....1A 5 3 First photoelectric lightcurves in two colors and omproved elements for V482 Persei and V651 Cassiopeiae. AGERER F. and LICHTENKNECKER D.
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.
2010ApJS..188..473N viz 15       D               1 832 10 The Chandra Variable Guide Star Catalog. NICHOLS J.S., HENDEN A.A., HUENEMOERDER D.P., et al.
1993yCat.3135....0C viz 14       D               1 252979 52 VizieR Online Data Catalog: Henry Draper Catalogue and Extension, published in Ann. Harvard Obs. 91-100 (1918-1925) CANNON A.J. and PICKERING E.C.
2017AJ....153..257O viz 16       D               1 10625 142 Comoving stars in Gaia DR1: an abundance of very wide separation comoving pairs. OH S., PRICE-WHELAN A.M., HOGG D.W., et al.
2018AJ....155..149B viz 16       D               1 9764 5 Fundamental properties of co-moving stars observed by Gaia. BOCHANSKI J.J., FAHERTY J.K., GAGNE J., 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.
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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