Results 71 to 80 of about 34,388 (227)
Winds from Nuclear Starbursts: Old Truths and Recent Progress on Superwinds
, 2004 I will discuss a few select aspects of the most common and best understood galactic-scale outflow -- starburst-driven superwinds, focusing on winds from nuclear starburst galaxies.
Strickland, David K.
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Current Star Formation in Post-Starburst Galaxies? [PDF]
, 2001 Radio continuum observations are a probe of star formation in galaxies, and are unaffected by dust extinction. Observations of the distant rich cluster Cl 0939+4713 have detected radio galaxies classified as post-starburst (``k+a'') on the basis of their
Miller, Neal A., Owen, Frazer N.
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Discovery of Large Molecular Gas Reservoirs in Post-Starburst Galaxies
, 2015 Post-starburst (or "E+A") galaxies are characterized by low H$\alpha$ emission and strong Balmer absorption, suggesting a recent starburst, but little current star formation.
French, K. Decker +7 more
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The role of E+A and post-starburst galaxies – I. Models and model results [PDF]
, 2009 ‘The definitive version is available at www3.interscience.wiley.com '. Copyright Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2009.14416.xDifferent compositions of galaxy types in the field in comparison to galaxy clusters as described by the ...
Falkenberg, M.A. +2 more
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Densitometry and Thermometry of Starburst Galaxies
, 2011 With a goal toward deriving the physical conditions in external galaxies, we present a survey of formaldehyde (H2CO) and ammonia (NH3) emission and absorption in a sample of starburst galaxies using the Green Bank Telescope. By extending well-established
Araya +13 more
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Nir Line Observations of Starburst Galaxies [PDF]
Symposium - International Astronomical Union, 1999 We have obtained images of the H2and Brγ emission lines in the galaxy interacting system NGC 3690 + IC 694. We have also obtained simultaneous H- and K-band spectra for three of its 2μm continuum peaks. The most detectable line emission is concentrated at the continuum peaks. Therefore, the emission lines as well as stellar absorption lines can be used
H. Sugai +4 more
openaire +1 more source
The Astrophysical Journal, 1989 New multiaperture 1.65 and 2.2 micron photometry has been obtained for the central region of 132 spirals exhibiting 2 orders of magnitude range in central 10-micron luminosity. This multiaperture photometry along with optical spectroscopy indicated that the high central 10-micron luminosity (about 1 billion solar luminosities) is powered by massive ...
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The JWST EXCELS Survey: Insights into the Nature of Quenching at Cosmic Noon
The Astrophysical JournalWe study 24 massive quiescent galaxies with $\mathrm{log}{{M}}_{* }/{{M}}_{\odot }\gt 10$ at 1
Maya Skarbinski +21 more
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Starbursts in Multiple Galaxy Mergers
The Astrophysical Journal, 2001 23 pages 16 figures,2000,ApJ,545 in press.
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Starburst Galaxies in Their Last Billion Years: An Hδ Absorption Line Selected Sample
The Astrophysical JournalIn this paper, we focus on the study of starburst galaxies in their final billion years. Our galaxy selection is based solely on the presence of the H δ absorption line, which permits the later evolution of starburst galaxies to be traced, coinciding ...
Shumei Wu +3 more
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