The class of hot B-type stars consists of various sub-groups among which we find the classical Be stars and the more exotic B[e] stars. Both
Category: hotstars
The Faculty of Science at the University of Potsdam in Germany and ASU entered into the agreement in June 2021 with the objective of conducting
Jiří Kubát and Brankica Kubátová from the Stellar Department of Astronomical Institute have published an article in which they deal in detail with the effect
Today, astrophysicists use highly sensitive instruments and register every year thousands of supernovae, dozens of gamma-ray bursts, and even sources of gravitational waves. Due to
How much depends the predicted mass-lost rate due stellar winds on the parameters of the star and how these calculated values correspond to the observed