Results 101 to 110 of about 11,425 (209)
Vlt/Pionier Imaging Of Red Supergiant Stars
PIONIER (Precision Integrated-Optics Near-infrared Imaging ExpeRiment) was the first 4-telescope instrument installed at the Very Large Telescope Interferometer (VLTI) in 2010. Benefiting from the multiple interferometric configurations available at the Cerro Paranal observatory, it can efficiently image stellar surfaces. With their large linear sizes,
openaire +1 more source
Grown-up stars physics with MATISSE
MATISSE represents a great opportunity to image the environment around massive and evolved stars. This will allow one to put constraints on the circumstellar structure, on the mass ejection of dust and its reorganization , and on the dust-nature and ...
Bendjoya, P +22 more
core +3 more sources
On the formation of a 33 solar-mass black hole in a low-metallicity binary
A $33\,M_\odot$ black hole (BH) was recently discovered in an 11.6-year binary only 590 pc from the Sun. The system, Gaia BH3, contains a $0.8\,M_\odot$ low-metallicity giant ($\rm [M/H]=-2.2$) that is a member of the ED-2 stellar stream.
Kareem El-Badry
doaj +1 more source
History of two mass loss processes in VY CMa. [PDF]
Quintana-Lacaci G +6 more
europepmc +1 more source
Binary Evolution and the Progenitor of SN 1987A
Since the majority of massive stars are members of binary systems, an understanding of the intricacies of binary interactions is essential for understanding the large variety of supernova types and sub-types. I therefore briefly review the basic elements
Flórez-Acosta, Jorge +1 more
core +1 more source
Red supergiants (RSGs) represent a late evolutionary stage of massive stars. Recent observations reveal that the observed luminosity range of RSGs in young open clusters is wider than expected from single-star evolution models.
Chen Wang +14 more
doaj +1 more source
Circumstellar dust as a solution to the red supergiant supernova progenitor problem
We investigate the red supergiant problem: the apparent dearth of Type IIP supernova progenitors with masses between 16 and 30 M_sun. Although red supergiants with masses in this range have been observed, none have been identified as progenitors in pre ...
Böhm-Vitense +45 more
core +1 more source
A New Approach to Identifying Red Supergiant Stars in Metal-poor Galaxies: A Case Study of NGC 6822
A complete sample of red supergiant (RSG) stars is important for studying their properties. Identifying RSGs in extragalactic fields first requires removing the Galactic foreground dwarfs.
Zhi-wen Li +3 more
doaj +1 more source
Spectroscopic evidence for a large spot on the dimming Betelgeuse. [PDF]
Alexeeva S +6 more
europepmc +1 more source
Spitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud
We present a catalog of 1750 massive stars in the Large Magellanic Cloud, with accurate spectral types compiled from the literature, and a photometric catalog for a subset of 1268 of these stars, with the goal of exploring their infrared properties.
A. Z. Bonanos +110 more
core +1 more source

