Upper limits on X-ray emission from two rotating radio transients

Monthly Notices of the Royal Astronomical Society

Volumn 400, Issue 3, 2009, Pages 1445-1450

  Kaplan, D L ^a   Esposito, P ^b,c   Chatterjee, S ^d   Possenti, A ^e   McLaughlin, M A ^f,g   Camilo, F ^h   Chakrabarty, D ⁱ   Slane, P O ^j  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b INAF IASF MILANO   (Italy)

^c INFN SEZIONE DI PAVIA   (Italy)

^d Department of Obstetrics Gynecology   (United States)

^e INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^f WEST VIRGINIA UNIVERSITY   (United States)

^g NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^h Och Spine at New York Presbyterian Hospitals   (United States)

ⁱ MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^j HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

more..

Author keywords

Pulsars: general; Stars: neutron; X rays: stars

Indexed keywords

LUMINANCE; NEUTRONS; PULSARS; TEMPERATURE; X RAY SCATTERING;

CCD IMAGING; CHANDRA; IMAGING SPECTROMETERS; NEUTRON STARS; PROPERTY; PULSARS: GENERAL; STARS: NEUTRONS; UPPER LIMITS; X-RAY EMISSION; X-RAY:STARS;

ELECTROMAGNETIC WAVE EMISSION;

EID: 71849095194     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15541.x     Document Type: Article

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