20 citations · 30 across the 2 of their papers we have counts for
3 papers
Toward Understanding The B[e] Phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429
A. S. Miroshnichenko, E. L. Chentsov, V. G. Klochkova +19
FS CMa type stars are a group of Galactic objects with the B[e] phenomenon. They exhibit strong emission-line spectra and infrared excesses, which are most likely due to recently f…
The 2006 hot phase of Romano's star (GR 290) in M33
R. F. Viotti, S. Galleti, R. Gualandi +4
Understanding the nature of the instabilities of LBVs is important to understand the late evolutionary stages of very massive stars. We investigate the long term, S Dor-type variab…
The identification of the long-period X-ray pulsar 1WGA J1958.2+323 with a Be-star/X-ray binary
G. L. Israel, S. Covino, V. F. Polcaro +1
We present the results of optical observations performed between May and September 1998 of the stars within the position error circle of the recently discovered 12min pulsating X-r…