V* HO Vel , the SIMBAD biblio

V* HO Vel , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:42:59


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Title First 3 Authors
1933AN....249..395L 104 10 Neue Veranderliche am Sudhimmel. LUYTEN W.J.
1976IBVS.1213....1S 96 2 Spectral information on new and known long-period and related variables and some new late-type emission-line stars. STEPHENSON C.B. and SANDULEAK N.
1978IBVS.1414....1K 312 5 63rd Name-list of variables stars. KHOLOPOV P.N., KUKARKINA N.P. and PEROVA N.B.
1988IRASP.C......0J viz 14       D               1 245223 ~ Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190 JOINT IRAS SCIENCE WORKING GROUP
2005IBVS.5613....1A 50 5 New GCVS data for selected volume III variables. ANTIPIN S.V., PASTUKHOVA E.N. and SAMUS N.N.
1993yCat.3170....0M viz 14       D               1 10927 ~ IRAS Point Sources of flux at 12 microns greater than flux at 25 microns and falling within about 7 degrees of the Galactic Plane McCONNELL D.J.
2017ARep...61...80S viz 16       D               7150 446 General catalogue of variable stars: Version GCVS 5.1 SAMUS N.N., KAZAROVETS E.V., DURLEVICH O.V., et al.
2018A&A...618A..58M 16       D               1 89645 72 Gaia Data Release 2. The first Gaia catalogue of long-period variable candidates. MOWLAVI N., LECOEUR-TAIBI I., LEBZELTER T., et al.
2019MNRAS.486.1907J viz 16       D               1 8966 183 The ASAS-SN catalogue of variable stars - II. Uniform classification of 412 000 known variables. JAYASINGHE T., STANEK K.Z., KOCHANEK C.S., et al.
2022ApJS..260...46I viz 17       D               1 65989 11 The OGLE Collection of Variable Stars: Nearly 66,000 Mira Stars in the Milky Way. IWANEK P., SOSZYNSKI I., KOZLOWSKI S., et al.
2023ApJS..264...20I viz 17       D               1 65989 1 A Three-dimensional Map of the Milky Way Using 66,000 Mira Variable Stars. IWANEK P., POLESKI R., KOZLOWSKI S., et al.
2023A&A...674A..15L viz 17       D               1 1720610 15 Gaia Data Release 3 The second Gaia catalogue of long-period variable candidates. LEBZELTER T., MOWLAVI N., LECOEUR-TAIBI I., et al.

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