Negative Search for a Counterpart to the Gamma-Ray Repeater Source 0525-66

Details Negative Search for a Counterpart to the Gamma-Ray Repeater Source 0525-66 Negative Search for a Counterpart to the Gamma-Ray Repeater Source 0525-66

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...448..623d&link_type=abstract

Astrophysical Journal v.448, p.623

Astronomy and Astrophysics

Astronomy

32

Gamma Rays: Bursts, Infrared: Ism: Lines And Bands, Ism: Individual Alphanumeric: N49, Ism: Individual Alphanumeric: 0525-66, Ism: Supernova Remnants

Scientific paper

Radio continuum, near-infrared [Fe II], H2, and Brγ, and optical Hα images of the supernova remnant N49 in the LMC, show a filamentary shell structure, characteristic of remnants in the adolescent or middle-aged phase of their evolution. No evidence is found in these images for any feature associated with the soft γ-ray repeater 0525-66 projected within the outline of this SNR. The nature of an X-ray hot spot located near the position of the γ-ray source remains uncertain, but the lack of emission at other wavelengths places significant limits on any nonthermal contribution to its radiation.

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