RL 104 , the SIMBAD biblio

RL 104 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:52:25


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Title First 3 Authors
1974AJ.....79.1406R 93 22 Second finding list of faint blue stars in the anticenter region of the Galaxy. RUBIN V.C., WESTPFAHL D. and TUVE M.
1978AJ.....83..162C 97 21 UBV photometry of faint blue stars near the galactic anticenter. CHROMEY F.R.
1979AJ.....84..534C 58 18 Spectral types for faint blue stars near the galactic anticenter. CHROMEY F.R.
2001PASP..113.1393L viz 119 3 A finding list of faint UV-bright stars in the galactic plane. VI. LANNING H.H. and MEAKES M.
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.
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.
2022MNRAS.511L..66W 44           X         1 3 5 Discovery of hot subdwarfs covered with helium-burning ash. WERNER K., REINDL N., GEIER S., et al.
2022A&A...658A..66W 1193     A D S   X C       27 7 7 Non-local thermodynamic equilibrium spectral analysis of five hot, hydrogen-deficient pre-white dwarfs. WERNER K., REINDL N., DORSCH M., et al.
2022A&A...662A..40C viz 17       D               2 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.
2023ApJS..269...32S 148       D     X         4 70 ~ The GW Vir Instability Strip in Light of New Observations of PG 1159 Stars: Discovery of Pulsations in the Central Star of A72 and Variability of RX J0122.9-7521. SOWICKA P., HANDLER G., JONES D., et al.
2024ApJS..271...21L viz 18       D               1 204 ~ He-rich Hot Subdwarf Stars Observed in Gaia DR3 and LAMOST DR7: Carbon and Nitrogen Abundances and Kinematics. LUO Y., NEMETH P., WANG K., et al.

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