... discovery of these new stars increases the number of known RCB stars in the LMC to ... These stars decline much more slowly and are cooler than the RCB stars. ... stars are unknown since there is no direct measurement of the distance to any ...
... stars are generally cool stars: M-type giants and supergiants for example, or carbon ... star" spectrum is a carbon-star template spectrum formed from optical, near-infrared ...
... stars in the Large Magellanic Cloud (LMC) using radiative transfer (RT) models of ... star from each of the bright and faint O-rich AGB populations found by earlier ...
... Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC . ... stars) locked in young stars is systematically high (књ10 per cent) within the central 15 pc and systematically lower outside ...
... stars hotter than about 3000 K effective temperature radiate like a hot blackbody at ... hotter stars are very close to the same in shape while the cooler K-type giant star ... This is a "hypergiant" star, a very massive somewhat evolved star. ...
... stars in the Small Magellanic Cloud (SMC), with accurate spectral types compiled ... stars in the Large Magellanic Cloud (LMC), finding that the brightest infrared ... stars among O and early-B stars in our SMC catalog, respectively, when compared to ...
... stars are hydrogen-deficient, carbon-rich, pulsating, post-asymptotic giant branch ... eight RCB stars, the RCB-like star DY Per, and the final-helium-flash star FG Sge ...
... Observations show that most stars are formed in multiple star systems and that many have planets. ... JWST Birth of Stars and Protoplanetary Systems theme goal is to unravel the birth and early evolution of stars, from infall on ...