X‐Ray Observations of SN 1006 withINTEGRAL-Reference-Cited by-同舟云学术

X‐Ray Observations of SN 1006 withINTEGRAL

Published:2006-06-10 Issue:1 Volume:644 Page:274-278
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Kalemci E.,Reynolds S. P.,Boggs S. E.,Lund N.,Chenevez J.,Renaud M.,Rho J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference31 articles.

1. Upper limits to the SN1006 multi-TeV gamma-ray flux from HESS observations

2. X‐Ray Synchrotron Emission from 10–100 TeV Cosmic‐Ray Electrons in the Supernova Remnant SN 1006

3. Radio to Gamma‐Ray Emission from Shell‐Type Supernova Remnants: Predictions from Nonlinear Shock Acceleration Models

4. Is the remnant of SN 1006 Crablike

5. Chenevez, J., Lund, N., Westergaard, N. J., Budtz-Joergensen, C., Kretschmar, P. & Walter, R. 2004, in The 5th INTEGRAL Workshop on the INTEGRAL Universe, ed. V. Schonfelder, G. Lichti, & C. Winkler, (Nordwijk: ESA), 837

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