Results 131 to 140 of about 11,425 (209)
Atmospheric Dynamics of Red Supergiant Stars
Thanks to their high-peak infrared luminosity, red supergiant (RSG) stars are fundamental tracers of galactic structure, efficiently probing regions of high interstellar extinction. To understand their properties is crucial and impacts a broad segment of Astrophysics.In this thesis, the answer to the principal questions about RSGs is addressed with ...
openaire +1 more source
Mass-loss Rate of Highly Evolved Stars in the Magellanic Clouds
Asymptotic giant branch stars (AGBs) and red supergiant stars (RSGs) exhibit significant mass-loss phenomena and are considered important sources of interstellar dust.
Jing Wen +5 more
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The Explosion and Progenitor Properties of Type IIP Supernovae Inferred from MESA and STELLA Modelling. [PDF]
Ricks W, Dwarkadas VV.
europepmc +1 more source
Supernova (SN) 2024ggi is a nearby Type II SN discovered by the Asteroid Terrestrial-impact Last Alert System, showing early flash-ionization features. The preexplosion images reveal a red supergiant progenitor with an initial mass of 10–17 M _⊙ . In the
Amar Aryan +4 more
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Imaging the subsurface architecture in porphyry copper deposits using local earthquake tomography. [PDF]
Comte D +8 more
europepmc +1 more source
With the ever faster cadence of untargeted surveys of the sky, the supernova (SN) community will capture a growing number of shock breakouts in red supergiant (RSG) stars in the coming years.
Dessart Luc, Jacobson-Galán Wynn V.
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Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities. [PDF]
Rosati P +39 more
europepmc +1 more source
We present deep James Webb Space Telescope near-infrared imaging to search for a quiescent or transient counterpart to FRB 20250316A, which was precisely localized with the CHIME Outriggers array to an area of 11 × 13 pc in the outer regions of NGC 4141 ...
Peter K. Blanchard +25 more
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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
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Supernovae and transients with circumstellar interaction. [PDF]
Fraser M.
europepmc +1 more source

