Results 91 to 100 of about 3,144 (170)
Boil-off of red supergiants: mass loss and type II-P supernovae
The mass loss mechanism of red supergiant stars is not well understood, even though it has crucial consequences for their stellar evolution and the appearance of supernovae that occur upon core-collapse.
Jim Fuller, Daichi Tsuna
doaj +1 more source
Inner Workings: A massive star dies without a bang, revealing the sensitive nature of supernovae. [PDF]
Croswell K.
europepmc +1 more source
2 supergiants and 2 hypergiants radio spectra
We present Herschel/HIFI spectra observed towards two Red Supergiants (NML Cyg, Betelgeuse) and two Yellow Hypergiants (AFGL2343, IRC+10420). The data focus on various transitions of 12CO, 13CO, ortho- and para- water, as well as some other bonus lines ...
Dominik, C. +2 more
core +1 more source
Red Supergiants—The Other Side of the H-R Diagram
Red supergiants are the largest stars known with some of the highest mass loss rates observed. They are the final stage in the evolution of the majority of massive stars.
Roberta M. Humphreys
doaj +1 more source
The Explosion and Progenitor Properties of Type IIP Supernovae Inferred from MESA and STELLA Modelling. [PDF]
Ricks W, Dwarkadas VV.
europepmc +1 more source
What Physical Factors Influence the Transformation between Blue Supergiants and Red Supergiants?
The post-main-sequence evolution of massive stars is highly sensitive to key stellar model parameters, particularly initial rotational velocity and metallicity.
Yun He +8 more
doaj +1 more source
Spectroscopic evidence for a large spot on the dimming Betelgeuse. [PDF]
Alexeeva S +6 more
europepmc +1 more source
Surface magnetic fields on giants and supergiants
After a short introduction to spectropolarimetry and the tecnics allowing for the detection of surface fields, I will review the numerous and various detections of magnetic fields at the surface of giant and supergiant stars.
Lebre, Agnès, Lebre, Agnès (5124368)
core +1 more source
Red supergiants and stellar evolution
We review the significant role played by red supergiants (RSGs) in stellar populations, and some challenges and questions they raise for theoretical stellar evolution. We present how metallicity and rotation modify the way stars go to
G. Meynet +4 more
core +1 more source
Red Supergiants as Supernova Progenitors
The inevitable fate of massive stars in the initial mass range of ≈8–30M⊙ in the red supergiant (RSG) phase is a core-collapse supernova (SN) explosion, although some stars may collapse directly to a black hole.
Schuyler D. Van Dyk
doaj +1 more source

