Scanner observations of main-sequence A and F stars.
Abstract
In order to understand the observed UB V colors of main-sequence A and F stars, and especially to understand the B - V gap observed for field stars and some clusters, we have made scanner observations of main-sequence stars with 0.20 < B - V < 0.45 in different clusters and with different Vr sin i. The results are given in Tables 2-7. Subject heading: spectrophotometry
- Publication:
-
The Astrophysical Journal Supplement Series
- Pub Date:
- December 1977
- DOI:
- 10.1086/190488
- Bibcode:
- 1977ApJS...35..461B