CD-43 14300 , the SIMBAD biblio

CD-43 14300 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.26CEST08:28:26


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Title First 3 Authors
1970BOTT....5..307D 146 8 A finding list of stars of spectral type A7 and earlier in regions at high galactic latitudes. IV. 3HLF4. DRILLING J.S. and PHILIP A.G.D.
1971AJ.....76.1072D 247 8 UBV photometry of early-type stars in 2 regions at high galactic latitudes. DRILLING J.S.
1993A&A...269..201D 3 3 Three stars at high galactic latitudes with peculiar helium abundances. DUFTON P.L., CONLON E.S., KEENAN F.P., et al.
2000CoSka..30...12Z 14 6 He, CNO abundances and (v sin i) in He-rich stars. ZBORIL M. and NORTH P.
2012MNRAS.427.2180N viz 15       D               1 181 117 A selection of hot subluminous stars in the GALEX survey – II. Subdwarf atmospheric parameters. NEMETH P., KAWKA A. and VENNES S.
2013MNRAS.431..240O viz 16       D               2 1287 13 The Edinburgh-Cape Blue Object Survey - III. Zone 2: galactic latitudes -30° > b > -40°. O'DONOGHUE D., KILKENNY D., KOEN C., et al.
2019A&A...621A..38G viz 17       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.
2019MNRAS.487.5922G viz 17       D               2 92 ~ Statistical analysis of roAp, He-weak, and He-rich stars. GHAZARYAN S., ALECIAN G. and HAKOBYAN A.A.
2019MNRAS.490.3158C viz 17       D               1 465834 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al.
2020MNRAS.499.5508S viz 17       D               1 1808 ~ A search for variable subdwarf B stars in TESS full frame images - I. Variable objects in the southern ecliptic hemisphere. SAHOO S.K., BARAN A.S., SANJAYAN S., et al.
2022A&A...662A..40C viz 18       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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