Discovery of the neutron star spin and a possible orbital period from the Be/X-ray binary IGR J05414-6858 in the LMC

Astronomy and Astrophysics

Volumn 542, Issue , 2012, Pages

  Sturm, R ^a   Haberl, F ^a   Rau, A ^a   Bartlett, E S ^b   Zhang, X L ^a   Schady, P ^a   Pietsch, W ^a   Greiner, J ^a   Coe, M J ^b   Udalski, A ^c  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^c UNIVERSITY OF WARSAW   (Poland)

Author keywords

Galaxies: individual: Large Magellanic Cloud; Stars: emission line, Be; Stars: neutron; X rays: binaries

Indexed keywords

ARCHIVAL DATA; BINARITY; LARGE MAGELLANIC CLOUDS; LIGHT CURVES; NEAR INFRARED; NEUTRON STARS; OPTICAL LIGHT; ORBITAL PERIODS; PHOTON INDEX; SMALL MAGELLANIC CLOUDS; STARS: EMISSION-LINE , BE; STARS: NEUTRONS; SWIFT SATELLITES; TARGET OF OPPORTUNITIES; X-RAY PROPERTIES; X-RAY SPECTRA; X-RAYS: BINARIES; XMM-NEWTON;

GALAXIES; NEUTRONS; X RAY ANALYSIS; X RAY SPECTROGRAPHS; X RAYS;

STARS;

EID: 84862278226     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219093     Document Type: Article

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