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In her PhD dissertation, Montserrat Armas Padilla focuses on the study of very faint X-ray binaries (VFXBs), which are a subgroup of X-ray binaries that display maximum luminosities several orders of magnitude lower than the ordinary well-studied X-ray binaries. She also analyses the only known VFXB harbouring a confirmed Black Hole (BH) accretor, namely Swift J1357.2-0933.

Event details of The spectral characteristics of X-ray binaries
Date 1 November 2013
Time 10:00 -11:00
Location Agnietenkapel

Mw. M. Armas Padilla, Subluminous X-ray Binaries.

Supervisor

Prof. M.B.M. van der Klis

Co-supervisor

Dr R.A.D. Wijnands

Agnietenkapel

Oudezijds Voorburgwal 229 - 231
1012 EZ Amsterdam

This event will be open to the public.