Hot subluminous stars at high galactic latitudes. I - Spectra and Stromgren photometry

Details Hot subluminous stars at high galactic latitudes. I - Spectra and Stromgren photometry Hot subluminous stars at high galactic latitudes. I - Spectra and Stromgren photometry

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...86...53m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 86, no. 1, Nov. 1990, p. 53-74.

Astronomy and Astrophysics

Astrophysics

85

Astronomical Photometry, Astronomical Spectroscopy, Hot Stars, Subdwarf Stars, Emission Spectra, Helium, Hydrogen, Main Sequence Stars

Scientific paper

Spectra of 92 stars selected from the Palomar-Green Catalog, most of them being hydrogen-rich (53) or helium-rich (21) hot subdwarfs, are presented. The rest belong to other spectral types, e.g. HBB or main-sequence B stars. Also presented is Stromgren photometry for 39 stars of the Palomer-Green Catalog, 29 of them belonging to the spectroscopically observed sample. The observations and their reduction are described and a spectral classification of the stars is given based on the spectra published here.

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