FIRST HARD X-RAY DETECTION OF THE NON-THERMAL EMISSION AROUND THE ARCHES CLUSTER: MORPHOLOGY AND SPECTRAL STUDIES WITHNuSTAR-Reference-Cited by-同舟云学术

FIRST HARD X-RAY DETECTION OF THE NON-THERMAL EMISSION AROUND THE ARCHES CLUSTER: MORPHOLOGY AND SPECTRAL STUDIES WITHNuSTAR

Published:2014-01-15 Issue:2 Volume:781 Page:107
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Krivonos Roman A.,Tomsick John A.,Bauer Franz E.,Baganoff Frederick K.,Barriere Nicolas M.,Bodaghee Arash,Boggs Steven E.,Christensen Finn E.,Craig William W.,Grefenstette Brian W.,Hailey Charles J.,Harrison Fiona A.,Hong JaeSub,Madsen Kristin K.,Mori Kaya,Nynka Melania,Stern Daniel,Zhang William W.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/781/i=2/a=107/pdf

Reference50 articles.

1. Discovery of X-ray flaring activity in the Arches cluster

2. Fe Kαline emission from the Arches cluster region – evidence for ongoing particle bombardment?

3. On winds and X-rays of O-type stars

4. Low-flux hard state of IE 1740.7-2942

5. Echoes of multiple outbursts of Sagittarius A⋆revealed byChandra

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