On the X-Ray Spectral Energy Distributions of Star-forming Galaxies: The 0.3–30 keV Spectrum of the Low-metallicity Starburst Galaxy VV 114-Reference-Cited by-同舟云学术

On the X-Ray Spectral Energy Distributions of Star-forming Galaxies: The 0.3–30 keV Spectrum of the Low-metallicity Starburst Galaxy VV 114

Published:2020-11-04 Issue:2 Volume:903 Page:79
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Garofali Kristen,Lehmer Bret D.^ORCID,Basu-Zych Antara,West Lacey A.^ORCID,Wik Daniel^ORCID,Yukita Mihoko,Vulic Neven^ORCID,Ptak Andrew^ORCID,Hornschemeier Ann

Funder

NASA

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abba2d/pdf

Reference116 articles.

1. X-rays across the galaxy population – I. Tracing the main sequence of star formation

2. A deepChandraobservation of the interacting star-forming galaxy Arp 299

3. Do sub-galactic regions follow the galaxy-wide X-ray scaling relations? The example of NGC 3310 and NGC 2276

4. Abundances of the elements: Meteoritic and solar

5. Star formation history and X-ray binary populations: the case of the Large Magellanic Cloud

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