1995/06/08 by A. M. Read, Read, A. M., T. J. Ponman +1
Engineering · Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics (astro-ph) #CCD and CMOS Imaging Sensors #Calibration and Measurement Techniques #Extreme ultraviolet lithography #FOS: Physical sciences #Flux (metallurgy) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Optics #Physics #ROSAT #Spiral galaxy #Supernova #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9506065
published in arXiv (Cornell University) (Cornell University) · 10 pages plus 5 figures, uuencoded encapsulated postscript file. Accepted for publication in MNRAS
arxiv created 1995/06/08 · openalex publication_date 1995/06/08 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Using data from the ROSAT Wide Field Camera all-sky survey, we have established upper limits to the extreme ultraviolet (EUV) flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish that the EUV flux escaping from galaxies does not contribute a major component of their bolometric luminosity, and in particular that it is very unlikely to be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band.