ON THE STELLAR CONTENT OF THE STARBURST GALAXY IC10 [PDF]
The Astrophysical Journal, 2009 7 pages, 4 figures, 1 table.
Sanna N +19 more
openaire +6 more sources
The equipartition magnetic field formula in starburst galaxies: accounting for pionic secondaries and strong energy losses [PDF]
, 2013 Equipartition arguments provide an easy way to find a characteristic scale for the magnetic field from radio emission, by assuming the energy densities in cosmic rays and magnetic fields are the same.
B. Lacki, R. Beck
semanticscholar +1 more source
Escape of Lyman continuum radiation from local galaxies - Detection of leakage from the young starburst Tol 1247-232 [PDF]
, 2013 Context. It has been suggested that the escape fraction of hydrogen ionizing photons (f(esc)) from galaxies is evolving with time, but the picture is far from clear.
E. Leitet +4 more
semanticscholar +1 more source
Dust Absorption and the Ultraviolet Luminosity Density at z ≈ 3 as Calibrated by Local Starburst Galaxies [PDF]
, 1999 We refine a technique to measure the absorption-corrected ultraviolet (UV) luminosity of starburst galaxies using rest-frame UV quantities alone and apply it to Lyman-limit U dropouts at z ≈ 3 found in the Hubble Deep Field (HDF).
G. Meurer, T. Heckman, D. Calzetti
semanticscholar +1 more source
The Astrophysical Journal, 1992 The use of SO and SO2 as probes of the dense interstellar medium in the nearby starburst galaxies NGC 253 and M82 is described. Emission in the 99.3 GHz 3(2) - 2(1) rotational transition of SO was detected in NGC 253 and possibly in M82, and upper limits are reported for emission in the 219.9 GHz 6(5) - 5(4) transition of SO and two lines of SO2.
Charles L. Bennett, S. J. Petuchowski
openaire +2 more sources
Winds of change: reionization by starburst galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2017 15 pages, 10 figures, Accepted for publication in MNRAS, comments ...
Sharma, M. +6 more
openaire +6 more sources
The cold gas content of post-starburst galaxies [PDF]
, 2013 Post-starburst galaxies, or E+A galaxies, are characterized by optical spectra showing strong Balmer absorption lines, indicating a young stellar population, and little or no emission lines, implying no active star formation.
M. Zwaan +3 more
semanticscholar +1 more source
A dominant population of optically invisible massive galaxies in the early Universe [PDF]
Nature, 2019 Our current knowledge of cosmic star-formation history during the first two billion years (corresponding to redshift z > 3) is mainly based on galaxies identified in rest-frame ultraviolet light1.
T. Wang +11 more
semanticscholar +1 more source
Age-Dating of Starburst Galaxies [PDF]
AIP Conference Proceedings, 2005 16 pages, 6 figures. Invited review talk. To be published in "The Evolution of Starbursts", ed. S. Huettemeister & E.
openaire +3 more sources
PROPERTIES OF NEARBY STARBURST GALAXIES BASED ON THEIR DIFFUSE GAMMA-RAY EMISSION [PDF]
, 2012 The physical relationship between the far-infrared and radio fluxes of star-forming galaxies has yet to be definitively determined. The favored interpretation, the “calorimeter model,” requires that supernova generated cosmic-ray (CR) electrons cool ...
T. Paglione, Ryan D. Abrahams
semanticscholar +1 more source