Ashok, N. M.; Bhatt, H. C.; Kulkarni, P. V.; Joshi, S. C.
(1984)
The Be stars as a class have been studied. JHK (1.2, 1.65, 2.2 μm) magnitudes for 55 Be stars are presented along with L (3.5 μm) magnitudes for 15 of them. For 20 Be stars the observations it is shown that the energy input ...