Results 1 to 10 of about 270,460 (312)
The State of the Molecular Gas in Post-starburst Galaxies [PDF]
The Astrophysical Journal, 2023 The molecular gas in galaxies traces both the fuel for star formation and the processes that can enhance or suppress star formation. Observations of the molecular gas state can thus point to when and why galaxies stop forming stars.
K. Decker French +9 more
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The role of E+A and post-starburst galaxies – II. Spectral energy distributions and comparison with observations [PDF]
, 2009 ‘The definitive version is available at www3.interscience.wiley.com '. Copyright Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2009.15036.xIn a previous paper, we have shown that the classical definition of E+A galaxies excludes a significant ...
Anders +59 more
core +4 more sources
Starbursts in multiple galaxy mergers [PDF]
The Astrophysical Journal, 2000 We numerically investigate stellar and gaseous dynamical evolution of mergers between five identical late-type disk galaxies with the special emphasis on star formation history and chemical evolution of multiple galaxy mergers.
Athanassoula E. +9 more
core +3 more sources
The Evolution of Starburst Galaxies [PDF]
, 2000 8 pages, 4 figures, to be published in proceedings of the MPIA workshop, "Modes of Star Formation and the Origin of Field Star Populations", ed. E.
Christopher J. Conselice
openalex +3 more sources
The Nature of Starburst Galaxies [PDF]
The Astrophysical Journal, 1996 Utilizing a large sample of infrared-selected starburst galaxies having optical images and long-slit spectra, we explore the interrelationships between the properties of starbursts and relate these properties to those of the "host" galaxy. We find that the half-light radius of the Hα-emitting region (re, Hα) enters into several correlations that ...
M. D. Lehnert, Timothy M. Heckman
openalex +2 more sources
Group-cluster merging and the formation of starburst galaxies [PDF]
, 1998 A significant fraction of clusters of galaxies are observed to have substructure, which implies that merging between clusters and subclusters is a rather common physical process of cluster formation. It still remains unclear how cluster merging affects
Barger A. J. +8 more
core +4 more sources
Proceedings of 8th European VLBI Network Symposium — PoS(8thEVN), 2007 15 pages, 19 figures, To appear in the proceedings of `The 8th European VLBI Network Symposium on New Developments in VLBI Science and Technology', ed. A. Marecki et al., held in Torun, Poland, on September 26-29, 2006 (Invited Review)
Muxlow, Tom +3 more
openaire +4 more sources
CH+(1-0) in a z~2.8 galaxy group: Probe of multi-phasic turbulent gas reservoirs [PDF]
EPJ Web of Conferences, 2022 Starburst galaxies at redshifts z~2 to 4 are among the most intensely star-forming galaxies in the universe. The way they accrete their gas to form stars at such high rates is still a controversial issue.
Vidal-García Alba +13 more
doaj +1 more source
ALCHEMI: Results from the ALMA Comprehensive High-resolution Extragalactic Molecular Inventory of NGC253 [PDF]
EPJ Web of Conferences, 2022 The star formation process in galaxies drives their evolution. The physical conditions which drive the star formation process in galaxies are studied using measurements of atomic and molecular species found in the dense has from which stars form in ...
Mangum Jeffrey G., Viti Serena
doaj +1 more source
KM3NeT/ARCA Sensitivity to Starburst Galaxies [PDF]
EPJ Web of Conferences, 2023 In this work, the expectations of the full detector KM3NeT/ARCA are presented for particular starburst galaxies signals. For the point-like search approach, we considered the most promising local starburst galaxies to be observed as point-like neutrino ...
Ambrosone A. +5 more
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