Infrared photometry of four relatively faint (8.5 ≤ V ≤ 11.0) early-type stars at high galactic latitude has been made in the J, H, K, L' 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.
|Number of pages||3|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publication status||Published - 01 Jan 1991|
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science