Results 91 to 100 of about 282,692 (200)
The z = 9.625 Cosmic Gems galaxy was a compact “blue monster” propelled by massive star clusters★
The recent discovery of five massive stellar clusters at z = 9.625 in the Cosmic Gems galaxy has raised the question about the formation mechanism of star clusters in the first 500 Myr after the Big Bang. We inferred the total stellar mass in clusters by
Vanzella E. +39 more
doaj +1 more source
I review the process of mass transfer in a binary system through a stellar wind, with an emphasis on systems containing a red giant. I show how wind accretion in a binary system is different from the usually assumed Bondi-Hoyle approximation, first as ...
A. A. Bonačić Marinović +69 more
core +1 more source
We present individual star formation histories (SFHs) of ∼3000 massive galaxies (log( M _* / M _⊙ ) > 10.5) from the Large Early Galaxy Astrophysics Census spectroscopic survey at a lookback time of ∼7 billion yr and quantify the population trends ...
Yasha Kaushal +15 more
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Galaxy And Mass Assembly: Stellar Mass Estimates
Accepted for publication in MNRAS. 35 pages; 21 figures including 6 in 2 appendices -- v2. corrected three extremely embarrassing typos in coauthors' names as they appeared in the arXiv metadata; manuscript text is ...
Taylor, E. +34 more
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Supernovae and Stellar Mass Loss [PDF]
AbstractType I supernovae can be modeled as the carbon deflagration of white dwarfs and Type II supernovae as the explosions of massive stars with hydrogen envelopes. The massive stars at the ends of their lives are expected to be red supergiants, which are observed to have slow, dense winds.
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Coevolution of Nuclear Star Clusters and Massive Black Holes: Extreme-mass-ratio Inspirals
We explore extreme-mass-ratio inspirals (EMRIs) in the coevolution of massive black holes (MBHs) and nuclear star clusters (NSCs), which host diverse stellar populations across a wide range of masses. The dynamics are simulated self-consistently with GNC
Fupeng Zhang, Pau Amaro Seoane
doaj +1 more source
15 pages incl. 4 figures (LaTeX, style files included); The figures are larger than in the 12 page review that is to appear in PASPC: Brown Dwarfs and Extrasolar Planets, R. Rebolo, M.R. Zapatero Osorio and E.
openaire +2 more sources
The stellar initial mass function [PDF]
Abstract The IMF UNIVERSALITY HYPOTHESIS cannot be discarded despite the existence of the CLUSTER IMF THEOREM. This means that the currently existing star-formation theory fails to describe the stellar outcome. The IGIMF THEOREM, however, predicts a variation of galaxy-wide IMFs in dependence of the galaxy's star-formation rate even if the IMF ...
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Whereas well-studied galaxies at cosmic noon are found to be baryon dominated within the effective radius, recent JWST observations of z ∼ 6–7 galaxies with stellar masses of only M _* ∼ 10 ^8−9 M _⊙ surprisingly indicate that they are dark matter ...
Anna de Graaff +2 more
doaj +1 more source
We investigate the cosmic evolution of the internal structure of massive early-type galaxies over half of the age of the Universe. We perform a joint lensing and stellar dynamics analysis of a sample of 81 strong lenses from the SL2S and SLACS surveys ...
Auger, Matthew W. +6 more
core +3 more sources

