SBSS 0941+558 , the SIMBAD biblio

SBSS 0941+558 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST08:05:14

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1984Afz....20...21M 131 26 The second Byurakan spectral sky survey. II. The results of the area centred on alpha = 09h 50m, delta = +55 00. MARKARIAN B.E. and STEPANIAN J.A.
1990AJ....100.1014M 144 73 High-redshift radio galaxies from Molonglo catalogue. McCARTHY P.J., KAPAHI V.K., VAN BREUGEL W., et al.
1990AJ....100.1028S 131 4 Accurate optical positions for 110 Byurakan objects and 24 blue stars from the "Second Byurakan spectral sky survey (II)". SEAL J., CHAVEZ D. and KOJOIAN G.
1997Ap.....40..101B 317 2 Spectral classification of stars in the Second Byurakan Sky Survey. I. BALAYAN S.K.
1999PASP..111.1099S 364 12 Spectroscopy of stellar-like objects contained in the second Byurakan survey. I. STEPANIAN J.A., CHAVUSHYAN V.H., CARRASCO L., et al.
2005RMxAA..41..155S viz 3230 23 The Second Byurakan Survey. General Catalogue. STEPANIAN J.A.
2016yCat....1.2035M viz 16       D               14271 ~ A Catalogue of Spectroscopically Identified White Dwarfs MCCOOK G.P. and SION E.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.
2023ApJS..264...17Z viz 17       D               4 31380 1 Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. ZHANG L.-Y., SU T., MISRA P., et al.
2023MNRAS.519..995L 844       D     X C F     18 19 ~ Origins of B-type stars at high Galactic latitudes based on abundances and kinematics. LIU Z., CUI W., ZHAO G., et al.

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