Results 111 to 120 of about 1,537 (221)

Prevalence of non-aromatic carbonaceous molecules in the inner regions of circumstellar envelopes. [PDF]

open access: yesNat Astron, 2020
Martínez L   +16 more
europepmc   +1 more source

The chemical composition of the circumstellar envelopes around yellow hypergiant stars

open access: yes, 2007
Context.The yellow hypergiant stars (YHGs) are extremely luminous and massive objects whose general properties are poorly known. Only two of this kind of star show massive circumstellar envelopes, IRC +10420 and AFGL 2343.
G. Quintana-Lacaci   +3 more
core   +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]

open access: yesAstrophys J, 2020
Santoro G   +15 more
europepmc   +1 more source

CONSTRAINTS ON THE GEOMETRY OF CIRCUMSTELLAR ENVELOPES: Optical Interferometric and. . .

open access: yes, 1997
We have obtained contemporaneous optical interferometry and spectropolarimetry of seven Be stars. The interferometry was done using both continuum and narrow Ha line Ðlters to observe the circumstellar envelope emission.
J. E. Bjorkman   +5 more
core  

86th Annual Meeting of the Meteoritical Society (2024)

open access: yes
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley   +1 more source

Molecular Line Studies of Circumstellar Envelopes

open access: yes, 1982
This dissertation addresses several problems in the study of the dusty, gaseous envelopes commonly found around highly evolved stars. Most of the objects observed are M or N giants and are typically long-period variables.
Jewell, Philip Ramer
core  

Dance to Demise—How Massive Stars May Form Dense Circumstellar Shells before Explosion

open access: yesThe Astrophysical Journal
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

Discontinuous Galerkin finite element method for the continuum radiative transfer problem inside axis-symmetric circumstellar envelopes

open access: yes
International audienceContext. The study of the continuum radiative transfer problem inside circumstellar envelopes is both a theoretical and numerical challenge, especially in the frequency-dependent and multi-dimensional case. While approximate methods
Faurobert, Marianne   +8 more
core   +1 more source

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