... with M > 10M is quite different from low mass stars, and what happens at M 100M 51 ... 52 The carbon-oxygen cores of low mass stars turn out to be degenerate at the moment ...

... orbit time) of binary neutron stars PSR1913+16 is explained by transformation of mass of stars into gravitational radiation ...

... that the enrichment of oxygen and nitrogen massive galaxies (and, therefore, active star formation) occurred in the past, and ... The use of "Lithium test" possible to find among the set of low-mass stars young brown dwarfs. ...

... Bondugin Тема: Hubble Finds That Even Massive Stars Just Fade Away Привет всем ... PR98-16 HUBBLE FINDS THAT EVEN MASSIVE STARS JUST FADE AWAY Pinpointing the rapidly ...

... collapse of a rapidly rotating core of a massive star and short gamma-ray burst are ... of a collapse of a core of a massive star the spinar is surrounded by the star's ...

... cores associated with Galactic high-mass star forming regions Pirogov, 1999 reveal ... This well-known high-mass star forming region demonstrates very strong HCN lines ...

... show extremely blue colours indicative of massive star formation, the rate at which ... as well, as e.g. cataclysmic variable stars (where mass accretion from a low-mass ...

... Fields of interest: hot massive stars, close binary systems: optical photometric and spectral observations, X-ray observations; ill-posed problems, X-ray astrophysics. ...

... The most massive stars (O-stars) can have masses up to 60 solar masses (even 100 solar masses seem possible). ... On the other side, the sequence is bounded by light-weight M-stars with masses down to 0.08 solar masses. ...

... Meet the Titans: Dust Disk Found Around Massive Star A new discovery has the potential to answer the longstanding question of ...