The Coronae of AR Lac
We observed the coronally active eclipsing binary AR Lac with the High Energy Transmission Grating on Chandra for a total of 97 ks, spaced over five orbits, at quadratures and conjunctions. Contemporaneous and simultaneous EUV spectra and photometry were also obtained with the Extreme Ultraviolet Ex...
Main Authors: | Huenemoerder, David P. (Contributor), Canizares, Claude R. (Contributor), Drake, Jeremy J. (Author) |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research (Contributor), Canizares, Claude (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2013-01-07T21:17:10Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
A 33 yr CONSTANCY OF THE X-RAY CORONAE OF AR Lac AND ECLIPSE DIAGNOSIS OF SCALE HEIGHT
by: Drake, Jeremy J., et al.
Published: (2015) -
HEATING IN AN EXTENDED ACCRETION DISK CORONA ALONG THE Z-PATTERN IN CYG X-2
by: Schulz, Norbert S., et al.
Published: (2010) -
X-RAY FLARES OF EV Lac: STATISTICS, SPECTRA, AND DIAGNOSTICS
by: Huenemoerder, David P., et al.
Published: (2015) -
X-RAY EMISSION AND CORONA OF THE YOUNG INTERMEDIATE-MASS BINARY theta(1) Ori E
by: Huenemoerder, David P., et al.
Published: (2010) -
X-Ray Spectroscopy of II Pegasi: Coronal Temperature Structure, Abundances, and Variability
by: Huenemoerder, David P., et al.
Published: (2013)