Results 11 to 20 of about 267,257 (315)

Theoretical Modeling of Starburst Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2001
36 pages, 16 figures, to be published in ApJ, July 20 ...
Kewley, Lisa   +4 more
openaire   +6 more sources

Are starburst galaxies proton calorimeters? [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
17 pages, 8 figures.
Xilu Wang (王夕露), Brian D Fields
openaire   +5 more sources

The evolutionary sequence of post-starburst galaxies [PDF]

open access: yes, 2017
© 2017 The Authors. There are multiple ways in which to select post-starburst galaxies in the literature. In this work, we present a study into how two well-used selection techniques have consequences on observable post-starburst galaxy parameters, such ...
Pimbblet, K. A.   +2 more
core   +5 more sources

Particle acceleration in the superwinds of starburst galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2018
Context. Starbursts are galaxies undergoing massive episodes of star formation. The combined effect of stellar winds from hot stars and supernova explosions creates a high-temperature cavity in the nuclear region of these objects. The very hot gas expands adiabatically and escapes from the galaxy creating a superwind which sweeps matter from the ...
A. L. Müller   +4 more
openaire   +8 more sources

Evolution Through the Post-starburst Phase: Using Post-starburst Galaxies as Laboratories for Understanding the Processes that Drive Galaxy Evolution [PDF]

open access: yesPublications of the Astronomical Society of the Pacific, 2021
Post-starburst (or “E+A”) galaxies trace the fastest and most dramatic processes in galaxy evolution. Recent work studying the evolution of galaxies through this phase has revealed insights on how galaxies undergo structural and stellar population ...
K. D. French
semanticscholar   +1 more source

The Compact Structures of Massive z ∼ 0.7 Post-starburst Galaxies in the SQuIGGL⃗E Sample [PDF]

open access: yes, 2022
We present structural measurements of 145 spectroscopically selected intermediate-redshift (z ∼ 0.7), massive (M ⋆ ∼ 1011 M ⊙) post-starburst galaxies from the SQuIGGL⃗E sample measured using wide-depth Hyper Suprime-Cam i-band imaging. This deep imaging
D. Setton   +11 more
semanticscholar   +1 more source

The star formation histories of z ∼ 1 post-starburst galaxies [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2020
We present the star formation histories of 39 galaxies with high-quality rest-frame optical spectra at 0.5 < z < 1.3 selected to have strong Balmer absorption lines and/or Balmer break, and compare to a sample of spectroscopically selected quiescent ...
V. Wild   +13 more
semanticscholar   +1 more source

COLDz: A High Space Density of Massive Dusty Starburst Galaxies ∼1 Billion Years after the Big Bang [PDF]

open access: yesAstrophysical Journal, 2020
We report the detection of CO(J = 2 → 1) emission from three massive dusty starburst galaxies at z > 5 through molecular line scans in the NSF’s Karl G. Jansky Very Large Array (VLA) CO Luminosity Density at High Redshift (COLDz) survey.
D. Riechers   +17 more
semanticscholar   +1 more source

Starburst galaxies strike back: a multi-messenger analysis with Fermi-LAT and IceCube data [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2020
Starburst galaxies, which are known as ‘reservoirs’ of high-energy cosmic-rays, can represent an important high-energy neutrino ‘factory’ contributing to the diffuse neutrino flux observed by IceCube. In this paper, we revisit the constraints affecting
A. Ambrosone   +5 more
semanticscholar   +1 more source

Extreme accretion events: TDEs and changing‐look AGN

open access: yesAstronomische Nachrichten, Volume 344, Issue 4, May 2023., 2023
Abstract We present a review of the topics of X‐ray stellar tidal disruption events (TDEs) and changing‐look active galactic nuclei (AGN). Stars approaching a supermassive black hole (SMBH) can be tidally disrupted and accreted. TDEs were first discovered in the X‐ray regime and appear as luminous, giant‐amplitude flares from inactive galaxies.
S. Komossa, D. Grupe
wiley   +1 more source

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