Results 81 to 90 of about 2,154,904 (218)
We present Very Large Array observations of 16 Type IIn and Type II-L supernovae (SNe IIn and SNe II-L) at ≈1000–7000 days after explosion, probing circumstellar matter (CSM) at distances >10 ^16 cm from the progenitor. At these radii, the data directly
Charles D. Kilpatrick +5 more
doaj +1 more source
The circumstellar matter in the Be + K binary KX and seen in the uv spectra [PDF]
KX And (HD 218393) belongs to well-known and often observed Be stars. The periodicity of spectroscopic characteristics as well as other observations led to the conclusion that the star is a peculiar interacting binary (Harmanec et al. 1980). The aim of this paper is to present the phase-dependent behaviour of the UV spectrum of the star.
openaire +1 more source
Evolution of the circumstellar disc of alpha Eri
3 pages ; to appear in the proceedings of the Sapporo meeting on active OB stars ; ASP Conference Series ; eds: S. Stefl, S. Owocki and A. OkazakiThe Halpha line emission formation region in the circumstellar disc of alpha Eri is: a) extended with a ...
Vinicius, M.M.F. +3 more
core +1 more source
SN 2022jox: An Extraordinarily Ordinary Type II SN with Flash Spectroscopy
We present high-cadence optical and ultraviolet (UV) observations of the Type II supernova (SN), SN 2022jox which exhibits early spectroscopic high-ionization flash features of H i , He ii , C iv , and N iv that disappear within the first few days after ...
Jennifer E. Andrews +22 more
doaj +1 more source
Detection of C60 in circumstellar environments
Buckminsterfullerene (C60) was recently discovered in the infrared spectra of a series of circumstellar envelopes. Given their remarkable stability, C60 and its derivatives are presumably able to survive during the envelope dispersion into the ...
Zhang, Y
core
The post-main-sequence evolution of massive stars involves phases of intense, often eruptive mass loss, including the B[e] supergiant phase. These hot stars are surrounded by cool, dense circumstellar disks that host complex chemistry, producing both ...
María Laura Arias +3 more
doaj +1 more source
Supernova interactions with aspherical circumstellar material
We present upgraded detailed numerical calculations of supernova (SN) interactions with significantly aspherical circumstellar matter (CSM), primarily formed as a disc or bipolar lobes.
Kurfürst P. +7 more
doaj +1 more source
Journal of Social Philosophy, Volume 55, Issue 4, Page 624-642, Winter 2024.
Luke Moffett
wiley +1 more source
We report C, N, Si, and Al–Mg isotope data for 39 presolar X silicon carbide (SiC) and four silicon nitride grains—a group of presolar grains that condensed in the remnants of core-collapse Type II supernovae (CCSNe)—isolated from the Murchison meteorite.
Nan Liu +5 more
doaj +1 more source
Can circumstellar interaction explain the strange light-curve features of Type Ib/c supernovae?
Context. The evolution and surrounding of the progenitors of stripped-envelope supernovae are still debated: some studies suggest single-star progenitors, but others prefer massive binary progenitors.
Andrea P. Nagy, Zsófia R. Bodola
core +1 more source

