Results 11 to 20 of about 271,838 (312)
Are starburst galaxies proton calorimeters [PDF]
Several starburst galaxies have been observed in the GeV and TeV bands. In these dense environments, gamma-ray emission should be dominated by cosmic-ray interactions with the interstellar medium ($p_{\rm cr}p_{\rm ism} \to \pi^{0} \to \gamma\gamma ...
Xilu Wang, B. Fields
semanticscholar +4 more sources
Starbursts in multiple galaxy mergers [PDF]
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
Studying the Interstellar Medium of H II/BCD Galaxies Using IFU Spectroscopy
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
Starburst radio galaxies: general properties, evolutionary histories and triggering [PDF]
In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of starburst radio galaxies in the context of scenarios for the triggering of the activity and the evolution of the host galaxies.
Almeida, C. Ramos +8 more
core +7 more sources
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
NIR Line Observations of Starburst Galaxies [PDF]
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
Hajime Sugai +4 more
openalex +2 more sources
COLDz: A High Space Density of Massive Dusty Starburst Galaxies ∼1 Billion Years after the Big Bang [PDF]
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]
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
KM3NeT/ARCA Sensitivity to Starburst Galaxies [PDF]
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
doaj +1 more source
Decomposition of the central structure of NGC 2273 in the NIR: A case study
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

