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

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

The Arches cluster is a young, densely packed massive star cluster in our Galaxy that shows a high level of star formation activity. The nature of the extended non-thermal X-ray emission around the cluster remains unclear. The observed bright Fe Kα line emission at 6.4 keV from material that is neut...

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Hlavní autoři: Krivonos, Roman A., Tomsick, John A., Bauer, Franz E., 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., Baganoff, Frederick K
Další autoři: MIT Kavli Institute for Astrophysics and Space Research
Médium: Článek
Jazyk:en_US
Vydáno: IOP Publishing 2015
On-line přístup:http://hdl.handle.net/1721.1/94544

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