We present the first 3D radiation hydrodynamics simulations of partially stripped ( ${M}_{{\rm{core}}}\sim 10{M}_{\odot }$ , M _env ∼ 0.1–1 M _⊙ ) yellow supergiant ( L ∼ 10 ^5 L _⊙ , T _eff ≈ 5000–8000 K) envelopes, constructed with Athena++ .
Jared A. Goldberg +3 more
doaj +1 more source
Molecules and Chemistry in Red Supergiants
The envelopes of Red Supergiants (RSGs) have a unique chemical environment not seen in other types of stars. They foster an oxygen-rich synthesis but are tempered by sporadic and chaotic mass loss, which distorts the envelope and creates complex outflow ...
Lucy M. Ziurys, Anita M. S. Richards
doaj +1 more source
Prevalence of non-aromatic carbonaceous molecules in the inner regions of circumstellar envelopes. [PDF]
Martínez L +16 more
europepmc +1 more source
Hα Emission among Evolved FGKM Stars: A Compendium from the Literature
Emission in the wings of the H α line among late-type giant stars occurs as a consequence of conditions in their chromospheres. Data from the literature have been used to document the incidence of H α emission among Population I giant stars as a function
Graeme H. Smith
doaj +1 more source
The Chemistry of Cosmic Dust Analogues from C, C<sub>2</sub>, and C<sub>2</sub>H<sub>2</sub> in C-Rich Circumstellar Envelopes. [PDF]
Santoro G +15 more
europepmc +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
Unconventional gas-phase preparation of the prototype polycyclic aromatic hydrocarbon naphthalene (C10H8) via the reaction of benzyl (C7H7) and propargyl (C3H3) radicals coupled with hydrogen-atom assisted isomerization. [PDF]
He C +9 more
europepmc +1 more source
Dance to Demise—How Massive Stars May Form Dense Circumstellar Shells before Explosion
We investigate the evolution of red supergiant (RSG) progenitors of core-collapse supernovae (SNe) with initial masses between 12 and 20 M _⊙ , focusing on the effects of enhanced mass loss due to pulsation-driven instabilities in their envelopes and ...
Sutirtha Sengupta +2 more
doaj +1 more source
Investigating Asymmetry Development from SiO to H2O Maser Regions in VX Sagittarii
Simultaneous very-long-baseline interferometry monitoring observations of H _2 O and SiO masers toward VX Sagittarii were conducted from 2014 February to 2019 January.
Dong-Hwan Yoon +4 more
doaj +1 more source

