ATTENZIONE! IL REPOSITORY E’ APERTO ESCLUSIVAMENTE ALL’IMMISSIONE DEI RAPPORTI TECNICI (COLLEZIONE 4.01). NON E’ POSSIBILE INSERIRE PRODOTTI IN TUTTE LE ALTRE COLLEZIONI, A CAUSA DI PROBLEMI TECNICI. THE REPOSITORY IS OPEN EXCLUSIVELY FOR THE SUBMISSION OF TECHNICAL REPORTS (COLLECTION 4.01). SUBMISSIONS TO ALL OTHER COLLECTIONS ARE TEMPORARILY UNAVAILABLE, DUE TO TECHNICAL ISSUES.
 

Hard X-ray Cataclysmic Variables

Journal
Date Issued
2020
Author(s)
•
•
Mukai, K.
•
Falanga, M.
•
DOI
Abstract
Among hard X-ray Galactic sources detected in the Swift and INTEGRAL surveys, those discovered as accreting white dwarf binaries have suprisingly boosted in number in the recent years. The majority are identified as magnetic Cataclysmic Variables of the Intermediate Polar type, suggesting this subclass as an important constituent of the Galactic population of X-ray sources. We here review and discuss the X-ray emission properties of newly discovered sources in the framework of an identification programme with the XMM-Newton satellite that increased the sample of this subclass by a factor of two.
Volume
66
Issue
5
Start page
1209
Uri
Url
Issn Identifier
0273-1177
Ads BibCode
2020AdSpR..66.1209D
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

1-s2.0-S0273117719306544-main.pdf

Description
[Administrators only]
Size

808.35 KB

Format

Adobe PDF

Checksum (MD5)

19d11c2f440a92e5195a382b84b919b9

Loading...
Thumbnail Image
Name

1909.06306.pdf

Description
preprint
Size

608.52 KB

Format

Adobe PDF

Checksum (MD5)

a1a74c708eabaf90f22fde5533676be1