Results 91 to 100 of about 2,154,904 (218)
Signs of a faint disc population at polluted white dwarfs [PDF]
Observations of atmospheric metals and dust discs around white dwarfs provide important clues to the fate of terrestrial planetary systems around intermediate-mass stars.
Rocchetto, M +3 more
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Observations of circumstellar disks
In this review I will present recent results obtained between 2005, which was the last “Be-stars” meeting in Sapporo, and 2010, on the observations of circumstellar disks around active hot stars.
Philippe Stee
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The carrier of the 21 μ m emission feature discovered in a handful of protoplanetary nebulae (PPNe) is one of the most intriguing enigmas in circumstellar chemistry.
Jian-Jie Qiu +9 more
doaj +1 more source
We report new medium-resolution spectroscopy covering the wavelength range from 0.6 to 2.4 μm, as well as multi-epoch, multi-wavelength photometry, of the Class I high-mass embedded young stellar object Mol 12 (IRAS 05373+2349). It is embedded (AV≃12) in
Mauricio Tapia +3 more
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Massive stars: the pre-supernova evolution of internal and circumstellar structure
We review new developments in the theory of massive stars and their circumstellar environments, considering the evolution from the main sequence to the supernova explosion.
Heger, A. (Max-Planck-Institut fuer Astrophysik, Garching (Germany)) +3 more
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Extreme Debris Disks: Insights into Violent Collisions in Planet Formation and Destruction
Debris disks are dusty structures around mature stars, primarily identified by infrared excesses in the stellar spectra. A subset, known as extreme debris disks (EDDs), exhibits stochastic infrared variability, believed to result from large-scale violent
Kate Y. L. Su +9 more
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The delay of shock breakout due to circumstellar material evident in most type II supernovae [PDF]
International audienceType II supernovae (SNe II) originate from the explosion of hydrogen-rich supergiant massive stars. Their first electromagnetic signature is the shock breakout (SBO), a short-lived phenomenon that can last for hours to days ...
Estévez, P. +122 more
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SN 2024abvb: A Type Icn Supernova in the Outskirts of Its Host Galaxy
We present multiband photometric and spectroscopic observations of supernova (SN) 2024abvb, which exhibits early-time prominent photoionized narrow emission lines of C II superposed on a blue continuum.
Maokai Hu +13 more
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Modeling the circumstellar interaction around SN 2004gq
Context. The relationship between the mass-loss history and final evolutionary stage of massive stars and the properties of the observable supernova (SN) is still under debate.
B. H. Pál, A. P. Nagy, T. Szalai
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Simulating the birth environment of circumstellar discs [PDF]
Circumstellar discs are the reservoirs of gas and dust that surround young stars and have the potential to become planetary systems. Their evolution will determine the time and material available to form planets.
Concha Ramirez, F.A.
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