NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Evidence for a corona of beta GeminorumA spectrometer was used on the satellite Copernicus to observe a chromospheric L alpha emission from the K0 giant beta Gem at 1218.4 A. This emission appears to be in the corona at temperatures near 260,000 deg K, since the ion it is identified with requires 77.4 eV to be produced.
Document ID
19750030101
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/181644
Authors
Gerola, H.
Shine, R. (Joint Institute for Laboratory Astrophysics Boulder, Colo., United States)
Mcclintock, W. (Johns Hopkins University Baltimore, Md., United States)
Linsky, J. L.
Henry, R. C.
Moos, H. W.
Date Acquired
August 8, 2013
Publication Date
November 1, 1974
Publication Information
Publication: Astrophysical Journal
Volume: 193
Subject Category
Astrophysics
Accession Number
75A14173
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.

Related Records

There are no records associated with this record.
No Preview Available