Home

About

Advanced Search

Browse by Discipline

Scientific Societies

E-print Alerts

Add E-prints

E-print Network
FAQHELPSITE MAPCONTACT US


  Advanced Search  

 
EXTRAGALACTIC ULTRAVIOLET BACKGROUND RADIATION Richard C. Henry
 

Summary: EXTRAGALACTIC ULTRAVIOLET BACKGROUND RADIATION
Richard C. Henry
Center for Astrophysical Sciences
Henry A. Rowland Department of Physics and Astronomy
The Johns Hopkins University
Baltimore, MD 21218
and
Space Astronomy and Astrophysics Group
Los Alamos National Laboratory
Jayant Murthy
Center for Astrophysical Sciences
Henry A. Rowland Department of Physics and Astronomy
The Johns Hopkins University
Baltimore, MD 21218
Cite as:
Henry, R. C., & Murthy, J., in "Extragalactic Background Radiation," ed. D. Calzetti, M. Fall,
M. Livio, and P. Madau, Cambridge: Cambridge Univ. Press, 51, 1995
Abstract. We describe observations of the cosmic background in the far ultraviolet. If the
Voyager upper limit on the cosmic diffuse ultraviolet background at 1100 at some locations is
accepted as correct, the spectrum of the high-galactic latitude background is most remarkable,

  

Source: Henry, Richard C.- Department of Physics and Astronomy, Johns Hopkins University

 

Collections: Physics