SN1987A
from
High-Energy Astrophysics: American and Soviet Perspectives/Proceedings
from the U.S.-U.S.S.R. Workshop on High-Energy Astrophysics (1991)
The SN1987A X-ray 15-105 keV flux as a funchtion of time according to the
Kvant HEXE observations. Each point corresponds to one observational day,
the errors correspond to one standard deviation. Three sigma upper limit
on the flux observed in May-June 1989 is presented.
|
|
Additions or Comments:
Have we left anything out? Is there something you would like to have added
to this page (a link to your own group's research page, for example...)?
|
IMAGES |
By Mission |
Stars |
Cataclysmic Variables |
X-ray Binaries |
Pulsars |
Supernova Remnants & Planetary Nebulae |
Galaxies |
Active Galactic Nuclei |
Clusters and Groups of Galaxies |
X-ray/gamma-ray Background & Deep Fields |
Solar System Objects |
Gamma Ray Bursts
HEASARC Home |
Observatories |
Archive |
Calibration |
Software |
Tools |
Students/Teachers/Public
Last modified: Thursday, 26-Jun-2003 13:48:44 EDT
| 
