Detection of new filamentary nebulosity near the giant nonthermal radio loop II

Details Detection of new filamentary nebulosity near the giant nonthermal radio loop II Detection of new filamentary nebulosity near the giant nonthermal radio loop II

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..78..169o&link_type=abstract

Astrophysics and Space Science, vol. 78, no. 1, Aug. 1981, p. 169-174.

Astronomy and Astrophysics

Astronomy

Astronomical Photography, H Alpha Line, Nebulae, Nonthermal Radiation, Radio Sources (Astronomy), Cosmic Dust, Filaments, Neutral Gases, Schmidt Cameras, Supernova Remnants

Scientific paper

IIIaJ survey plates from the 1.2 m SRC Schmidt are high-contrast copied in search of nebulosity at high galactic latitudes in the vicinity of the giant radio loop II. Some filamentary nebulosity, possible reflection, is detected for certain. It is pointed out that the reflection nebulosity has its filaments elongated in a direction approximately parallel to Loop II although it is a considerable angular distance away from the main radio ridge. If it is reflection nebulosity, however, it may be only a small section of a much larger complex of filaments of neutral gas and dust. It is thought that this larger nebula may be undetected in the present survey because it has no bright stars to illuminate it.

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