TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
TV Cassiopeia (TV Cas) is a well-known eclipsing Algol-type binary comprising a B9V primary and F7 IV secondary in an orbit with a period of 1.81 days, together with a purported low-mass companion in a wide orbit. Despite the considerable attention TV Cas has received in optical and UV bands, no X-r...
Main Authors: | Yang, Jun, Drake, Jeremy J., Wik, Daniel R., Laycock, Silas G. T. |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Published: |
MDPI AG
2020
|
Online Access: | https://hdl.handle.net/1721.1/124964 |
Similar Items
-
The unusual broad-band X-ray spectral variability of NGC 1313 X-1 seen with XMM–Newton, Chandra , and NuSTAR
by: Walton, DJ, et al.
Published: (2021) -
THE XMM-NEWTON /EPIC X-RAY LIGHT CURVE ANALYSIS OF WR 6
by: Ignace, R., et al.
Published: (2015) -
NGC 2992 IN AN X-RAY HIGH STATE OBSERVED BY XMM-NEWTON : RESPONSE OF THE RELATIVISTIC Fe Kα LINE TO THE CONTINUUM
by: Shu, X. W., et al.
Published: (2015) -
Disk-dominated States of 4U 1957+11: Chandra, XMM-Newton, and RXTE Observations of Ostensibly the Most Rapidly Spinning Galactic Black Hole
by: Nowak, Michael A., et al.
Published: (2012) -
THE GAS DYNAMICS OF NGC 4472 REVEALED BY XMM-NEWTON
by: Kraft, Ralph P., et al.
Published: (2015)