Results 21 to 30 of about 5,548,804 (305)
, 2023 In the hierarchical view of star formation, giant molecular clouds (GMCs) undergo fragmentation to form small-scale structures made up of stars and star clusters.
Turner, Jordan A;Dale, Daniel A;Lilly, James;..., Hsi-An Pan et al.
core +1 more source
Formation of the first stars [PDF]
Proceedings of 11th Symposium on Nuclei in the Cosmos — PoS(NIC XI), 2005 Review, revised version; now in print, Rep. Prog. Phys. (2013), 52 pages, 14 figures (for high-resolution, please see the journal)
openaire +6 more sources
Redshift distribution of gamma-ray bursts and star formation rate [PDF]
, 2006 Aims. The redshift distribution of gamma-ray bursts collected in the BATSE Catalog is compared with the star formation rate.We aim to clarify the accordance between them. We also study the case of comoving number density of bursts monotonously increasing
Bagoly, Zsolt +19 more
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Massive star and star cluster formation [PDF]
Proceedings of the International Astronomical Union, 2006 AbstractI review the status of massive star formation theories: accretion from collapsing, massive, turbulent cores; competitive accretion; and stellar collisions. I conclude the observational and theoretical evidence favors the first of these models.
openaire +2 more sources
Gas, star formation and quenching in galaxy clusters and groups [PDF]
, 2019 I will review our current knowledge of the link between the star formation activity+quenching and the gas availability and removal as a function of galaxy environment focusing on galaxy clusters and groups.
POGGIANTI, Bianca Maria +1 more
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Modeling Two First Hydrostatic Core Candidates Barnard 1b-N and 1b-S
The Astrophysical Journal, 2023 A first hydrostatic core (FHC) is proposed to form after the initial collapse of a prestellar core, as a seed of a Class 0 protostar. FHCs are difficult to observe because they are small, compact, embedded, and short lived.
Hao-Yuan Duan +3 more
doaj +1 more source
Dust transport in envelopes of disk-embedded planets
Astronomy & AstrophysicsPlanets embedded in protoplanetary disks accrete solids through their gaseous envelopes. The spatial distribution of these dust particles inside the envelopes of disk-embedded planets is poorly known.
Kuwahara Ayumu, Lambrechts Michiel
doaj +3 more sources
Triple Spiral Arms of a Triple Protostar System Imaged in Molecular Lines
The Astrophysical Journal, 2023 Most stars form in multiple-star systems. For a better understanding of their formation processes, it is important to resolve the individual protostellar components and the surrounding envelope and disk material at the earliest possible formation epoch ...
Jeong-Eun Lee +11 more
doaj +1 more source
The volumetric star formation law in nearby galaxies [PDF]
, 2022 Star formation laws are empirical relations between the cold gas (HI+H$_2$) content of a galaxy and its star formation rate (SFR), being crucial for any model of galaxy formation and evolution.
Bacchini, C. +5 more
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Star clusters in unperturbed spiral galaxies [PDF]
, 2008 Stars do not form in isolation, they form in groups known as star clusters. Star clusters are seen in a wide range of galaxies and environments. Their presence reveals the history of the host galaxy and the processes of its star formation.
Mora, Marcelo D.
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