Kameswara Rao, N; Ashok, N. M; Kulkarni, P. V
(Astronomical Society of India, 1981-06)
Observations of HR 2947 show that it is fainter by 0.3 mag in V compared to the magnitude listed by Cowley et al. (1969). The energy distribution from 1565 Armstrong to 1.25 micro is similar to that of a B5 III star and ...