A new super-soft X-ray source in the Small Magellanic Cloud: Discovery of the first Be/white dwarf system in the SMC?

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Sturm, R ^a   Haberl, F ^a   Pietsch, W ^a   Coe, M J ^b   Mereghetti, S ^c   La Palombara, N ^c   Owen, R A ^d   Udalski, A ^e  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^c INAF IASF MILANO   (Italy)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e UNIVERSITY OF WARSAW   (Poland)

Author keywords

galaxies: individual: SMC; galaxies: stellar content; stars: emission line, Be; white dwarfs; X rays: binaries

Indexed keywords

GALAXIES: INDIVIDUAL: SMC; GALAXIES: STELLAR CONTENT; STARS: EMISSION-LINE, BE; WHITE DWARFS; X-RAYS: BINARIES;

ELECTRON SOURCES; GALAXIES; X RAY ANALYSIS; X RAY APPARATUS; X RAY SPECTROGRAPHS; X RAYS;

STARS;

EID: 84855697237     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117789     Document Type: Article

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