Zobrazeno 1 - 10
of 57
pro vyhledávání: '"Free-fall time"'
Autor:
Mitsuru Kokubo, Takeo Minezaki
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 491:4615-4633
We examine the long-term optical/near-infrared (NIR) flux variability of a "changing-look" active galactic nucleus (AGN) Mrk 590 between 1998 and 2007. Multi-band multi-epoch optical/NIR photometry data from the SDSS Stripe 82 database and the Multic
Akademický článek
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Publikováno v:
Monthly Notices of the Royal Astronomical Society. 473:4220-4241
Star formation in a filamentary infrared dark cloud (IRDC) is simulated over a dynamic range of 4.2 pc to 28 au for a period of $3.5\times 10^5$ yr, including magnetic fields and both radiative and outflow feedback from the protostars. At the end of
Autor:
V. V. Zhuravlev
Dust is the usual minor component of the interstellar medium. Its dynamic role in the contraction of the diffuse gas into molecular clouds is commonly assumed to be negligible because of the small mass fraction, $f \simeq 0.01$. However, as shown in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a2c94f055f08fe0a904eaf2d5239e97
We investigate how the properties of Galactic giant molecular clouds (GMCs) and their denser substructures (clumps) correlate with the local star formation rate. We trace clouds using the $^{12}$CO(3-2) transition, as observed by the CO High Resoluti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::05d610c9389eb11dd8654e3b914ecde6
Autor:
Genevieve Parmentier
Publikováno v:
The Astrophysical Journal. 893:32
The presence of a volume density gradient in molecular clumps allow them to raise their star formation rate compared to what they would experience were their gas uniform in density. This higher star formation rate yields in turn a higher value for th
Autor:
Jiayi Sun, Antonio Usero, Kathryn Kreckel, Mélanie Chevance, Miguel Querejeta, Dyas Utomo, Adam K. Leroy, Guillermo A. Blanc, Eve C. Ostriker, Andreas Schruba, Erik Rosolowsky, Frank Bigiel, Karin Sandstrom, Cinthya N. Herrera, Alexander P. S. Hygate, Jérôme Pety, Eva Schinnerer, J. M. Diederik Kruijssen, Eric Emsellem
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 861 (2), pp.L18. ⟨10.3847/2041-8213/aacf8f⟩
The Astrophysical journal letters, 2018, 861 (2), pp.L18. ⟨10.3847/2041-8213/aacf8f⟩
The Astrophysical Journal
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 861 (2), pp.L18. ⟨10.3847/2041-8213/aacf8f⟩
The Astrophysical journal letters, 2018, 861 (2), pp.L18. ⟨10.3847/2041-8213/aacf8f⟩
The Astrophysical Journal
We estimate the star formation efficiency per gravitational free fall time, $\epsilon_{\rm ff}$, from observations of nearby galaxies with resolution matched to the typical size of a Giant Molecular Cloud. This quantity, $\epsilon_{\rm ff}$, is theor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bacc5f0d636d45828fe834899476b93
Autor:
Blakesley Burkhart
Stars form in supersonic turbulent molecular clouds that are self-gravitating. We present an analytic determination of the star formation rate (SFR) in a gravoturbulent medium based on the density probability distribution function of molecular clouds
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::60cee6f5cd089188a73e575c49e1bc76
We present a model for the temporal variability of long gamma-ray bursts during the prompt phase (the highly variable first 100 seconds or so), in the context of a magnetically arrested disk (MAD) around a black hole. In this state, sufficient magnet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2598f4f5b1618757dc4aec8aa98064aa
http://arxiv.org/abs/1606.01572
http://arxiv.org/abs/1606.01572
Autor:
S. V. Anathpindika
Publikováno v:
Astronomy & Astrophysics. 504:451-460
In this second paper of the sequel of two papers, we further investigate the problem of molecular cloud (MC) collision. Anathpindika (2009) (hereafter paper I) considered highly supersonic cloud collisions and examined the effect of bending and shear