PB 3950 , the SIMBAD biblio

PB 3950 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST19:40:10


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Title First 3 Authors
1977A&AS...28..123B viz 4516 49 A search for faint blue stars in high galactic latitudes. I. Nine PSS fields near the North Galactic Pole. BERGER J. and FRINGANT A.M.
2007ApJ...671.1708B viz 15       D               396 76 Hypervelocity stars. III. The space density and ejection history of main-sequence stars from the Galactic Center. BROWN W.R., GELLER M.J., KENYON S.J., et al.
2010AJ....139...59B viz 15       D               1 912 69 Velocity dispersion profile of the Milky Way halo. BROWN W.R., GELLER M.J., KENYON S.J., et al.
2012ApJ...751...55B viz 15       D               1 969 48 MMT hypervelocity star survey. II. Five new unbound stars. BROWN W.R., GELLER M.J. and KENYON S.J.
2015MNRAS.448.2260G viz 16       D               1 32939 53 A photometric selection of white dwarf candidates in Sloan Digital Sky Survey Data Release 10. GENTILE FUSILLO N.P., GANSICKE B.T. and GREISS S.
2017A&A...600A..50G viz 16       D               5613 59 The population of hot subdwarf stars studied with Gaia. I. The catalog of known hot subdwarf stars. GEIER S., OSTENSEN R.H., NEMETH P., et al.
2019A&A...621A..38G viz 16       D               1 39805 85 The population of hot subdwarf stars studied with Gaia. II. The Gaia DR2 catalogue of hot subluminous stars. GEIER S., RADDI R., GENTILE FUSILLO N.P., et al.
2020A&A...635A.193G viz 16       D               2 6177 44 The population of hot subdwarf stars studied with Gaia. III. Catalogue of known hot subdwarf stars: Data Release 2. GEIER S.
2021ApJS..256...28L viz 17       D               1 2206 16 Hot subdwarf atmospheric parameters, kinematics, and origins based on 1587 hot subdwarf stars observed in Gaia DR2 and LAMOST DR7. LUO Y., NEMETH P., WANG K., et al.
2022A&A...662A..40C viz 17       D               1 62976 9 The population of hot subdwarf stars studied with Gaia. IV. Catalogues of hot subluminous stars based on Gaia EDR3. CULPAN R., GEIER S., REINDL N., et al.

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