Infrared observations of high galactic latitude early-type stars

Details Infrared observations of high galactic latitude early-type stars Infrared observations of high galactic latitude early-type stars

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249..336f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, March 15, 1991, p. 336-338. SERC-supported researc

Astronomy and Astrophysics

Astronomy

4

B Stars, Early Stars, Infrared Photometry, Main Sequence Stars, Galactic Structure, Infrared Astronomy Satellite, Spectral Energy Distribution, Stellar Atmospheres

Scientific paper

Infrared photometry of four relatively faint (V = 8.5 - 11.0) early-type stars at high galactic latitude has been made in the J, H, K, L-prime and narrow-band M wavelengths. This has been combined with previously published ultraviolet and visible observations to enable a comparison with LTE model atmosphere fluxes. The results imply that at least three of the stars are normal main-sequence B-stars at large distances from the galactic plane.

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