Abstract
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.
Original language | English |
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Pages (from-to) | 336-338 |
Number of pages | 3 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 249 |
Issue number | 2 |
Publication status | Published - 01 Jan 1991 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science