VLT and Suzaku observations of the Fermi pulsar PSR J1028-5819

Astronomy and Astrophysics

Volumn 543, Issue , 2012, Pages

  Mignani, R P ^a,b   Razzano, M ^c,d,i   Esposito, P ^e   De Luca, A ^f,g   Marelli, M ^g,h   Oates, S R ^a   Saz Parkinson, P ⁱ  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF ZIELONA GÓRA   (Poland)

^c INFN SEZIONE DI PISA   (Italy)

^d UNIVERSITY OF PISA   (Italy)

^e INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^f INAF IASF MILANO   (Italy)

^g INFN SEZIONE DI PAVIA   (Italy)

^h UNIVERSITY OF INSUBRIA   (Italy)

ⁱ UNIVERSITY OF CALIFORNIA SANTA CRUZ   (United States)

Author keywords

Gamma rays: stars; Pulsars: individual: PSR J1028,5819; Stars: neutron; X rays: stars

Indexed keywords

ABSORPTION COLUMN DENSITY; CHANDRA; DIFFUSE EMISSION; FLUX LIMITS; GAMMA RAYS: STARS; HIGH SPATIAL RESOLUTION; HYDROGEN COLUMN DENSITY; MULTI-WAVELENGTH STUDY; NEUTRON STARS; OPTICAL BRIGHTNESS; OPTICAL EMISSIONS; OPTICAL IMAGE; OPTICAL OBSERVATIONS; POTENTIAL TARGETS; POWER-LAW; PULSAR WIND NEBULAE; PULSARS: INDIVIDUALS; ROTATIONAL ENERGY-LOSS; SPECTRAL INDICES; SPIN-DOWN; STARS: NEUTRONS; SURFACE BRIGHTNESS; VERY LARGE TELESCOPE; X RAY SPECTRUM; X RAYS: STARS; XMM-NEWTON;

ENERGY DISSIPATION; GAMMA RAYS; GEOMETRICAL OPTICS; LIGHT EMISSION; OPTICAL TELESCOPES; X RAYS;

STARS;

EID: 84863759859     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201218869     Document Type: Article

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