Spectroscopic evidence for a 5.4 minute orbital period in HM cancri

Astrophysical Journal Letters

Volumn 711, Issue 2 PART 2, 2010, Pages

  Roelofs, Gijs H A ^a   Rau, Arne ^b,c   Marsh, Tom R ^d   Steeghs, Danny ^d   Groot, Paul J ^e   Nelemans, Gijs ^e  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^d UNIVERSITY OF WARWICK   (United Kingdom)

^e RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

Author keywords

Binaries: close; Gravitational waves; Stars: individual (HM Cancri, V407 Vulpeculae); X rays: binaries

Indexed keywords

EID: 77749336411     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/711/2/L138     Document Type: Article

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