Are starburst galaxies proton calorimeters? [PDF]
Monthly Notices of the Royal Astronomical Society, 2017 17 pages, 8 figures.
Xilu Wang (王夕露), Brian D Fields
openaire +4 more sources
The evolutionary sequence of post-starburst galaxies [PDF]
, 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
Studying the Interstellar Medium of H II/BCD Galaxies Using IFU Spectroscopy
Advances in Astronomy, 2013 We review the results from our studies, and previous published work, on the spatially resolved physical properties of a sample of H ii/BCD galaxies, as obtained mainly from integral-field unit spectroscopy with Gemini/GMOS and VLT/VIMOS. We confirm that,
Patricio Lagos, Polychronis Papaderos
doaj +2 more sources
The Evolution of Post-Starburst Galaxies from $z\sim1$ to the Present [PDF]
, 2016 Post-starburst galaxies are in the transitional stage between blue, star-forming galaxies and red, quiescent galaxies, and therefore hold important clues for our understanding of galaxy evolution.
Ho, Shirley +3 more
core +2 more sources
Evolution Through the Post-starburst Phase: Using Post-starburst Galaxies as Laboratories for Understanding the Processes that Drive Galaxy Evolution [PDF]
Publications 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]
, 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]
Monthly 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]
Astrophysical 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]
Monthly 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
Decomposition of the central structure of NGC 2273 in the NIR: A case study
Astronomische Nachrichten, Volume 344, Issue 10, December 2023., 2023 Abstract The Seyfert 2 galaxy NGC 2273 is a prime target to explore how active nuclei can be fed. It has a star‐forming innermost nuclear ring with a radius of 0.33kpc from where material may be funneled to the supermassive black hole in its center. In this article, we discuss high‐resolution adaptive optics aided JHKs images of NGC 2273 taken with the
L. Schey +13 more
wiley +1 more source