A likely optical counterpart of the G292.0+1.8 pulsar wind nebula

Astronomy and Astrophysics

Volumn 492, Issue 3, 2008, Pages 805-814

  Zharikov, S V ^a   Shibanov, Yu A ^b   Zyuzin, D A ^b,c   Mennickent, R E ^d   Komarova, V N ^e  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^b IOFFE INSTITUTE   (Russian Federation)

^c Academical Physical Technical University   (Russian Federation)

^d UNIVERSITY OF CONCEPCIÓN   (Chile)

^e RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

Author keywords

Stars: neutron; Stars: pulsars: general; Stars: pulsars: individual: G292.0+1.8

Indexed keywords

FLUXES;

BAND SPECTRUMS; CENTER POSITIONS; COMPACT TORUS; DIRECT IMAGING; INTERSTELLAR EXTINCTIONS; MAJOR AXIS; MULTI WAVELENGTHS; OPTICAL BANDS; OPTICAL COUNTERPARTS; OPTICAL FLUXES; OPTICAL OBJECTS; OPTICAL OBSERVATIONS; OPTICAL SOURCES; PHYSICAL REGIONS; PULSAR WIND NEBULAE; SPATIAL RESOLUTIONS; SPECTRAL PROPERTIES; STARS: NEUTRON; STARS: PULSARS: GENERAL; STARS: PULSARS: INDIVIDUAL: G292.0+1.8; SUPERNOVA REMNANTS; TORUS REGIONS;

STARS;

EID: 57649228002     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810429     Document Type: Article

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