Observational and theoretical constraints for an Hα-halo around the Crab nebula

Astronomy and Astrophysics

Volumn 497, Issue 1, 2009, Pages 167-176

  Tziamtzis, A ^a   Schirmer, M ^b,c   Lundqvist, P ^a   Sollerman, J ^a  

^a ALBANOVA UNIVERSITY CENTER   (Sweden)

^b ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^c UNIVERSITY OF BONN   (Germany)

Author keywords

Ism: Supernova remnants; Stars: Supernovae: Individual: SN1054

Indexed keywords

COLLISIONAL EXCITATIONS; CONSTANT DEGREES; CONSTANT TEMPERATURES; CRAB NEBULAS; DE EXCITATIONS; DENSITY PROFILES; EMISSION SPECTRUMS; ERROR BARS; EXTENDED TARGETS; GAS MOTIONS; HIGH VELOCITIES; IONISATION; ISM: SUPERNOVA REMNANTS; POWER LAWS; PSF MODELS; RECOMBINATION EMISSIONS; RESEARCH AREAS; SHELL MODELS; SPECTROSCOPIC DETECTIONS; STARS: SUPERNOVAE: INDIVIDUAL: SN1054; SUPERNOVA REMNANTS; SURFACE BRIGHTNESS; TYPE II;

EMISSION SPECTROSCOPY; LEAKAGE (FLUID); OPTICAL INSTRUMENTS; OPTICAL TELESCOPES; OPTICAL TRANSFER FUNCTION; SCATTERING; STARS; TELESCOPES;

SHELLS (STRUCTURES);

EID: 63849230817     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811385     Document Type: Article

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