Soft X-ray survey of the Large Magellanic Cloud

Details Soft X-ray survey of the Large Magellanic Cloud Soft X-ray survey of the Large Magellanic Cloud

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196l..15r&link_type=abstract

Astrophysical Journal, vol. 196, Feb. 15, 1975, pt. 2, p. L15-L18.

Computer Science

Sound

15

Background Radiation, Magellanic Clouds, Radiant Flux Density, Rocket Sounding, X Ray Astronomy, Diffuse Radiation, Galactic Clusters, Galactic Radiation, X Ray Absorption

Scientific paper

A soft X-ray survey (0.15-1.5 keV) of the Large Magellanic Cloud (LMC) during a sounding rocket flight, reveals possible emission from the centrally located barlike structure. No evidence was seen for absorption of the soft X-ray 'background' in the direction of the LMC. Both of these observations support the hypothesis of a local production of the soft X-ray background.

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