Faint, nebulous filaments, 2000 PC diameter, around the 30 Doradus nebula

Details Faint, nebulous filaments, 2000 PC diameter, around the 30 Doradus nebula Faint, nebulous filaments, 2000 PC diameter, around the 30 Doradus nebula

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....75..127m&link_type=abstract

Astronomy and Astrophysics, vol. 75, no. 1-2, May 1979, p. 127-132.

Astronomy and Astrophysics

Astrophysics

43

Magellanic Clouds, Nebulae, Astronomical Photography, Hydrogen Clouds

Scientific paper

A 5h exposure of the Large Magellanic Cloud at H alpha + (N II) has been printed at high contrast and through a mask that filters out information at low spatial frequencies. The consequences are that many filaments of extremely faint nebulosity over a region, about 2000 pc diameter, surrounding the 30 Doradus nebula are revealed and their relationship to the brighter central filaments demonstrated. All the nebulous ridges, the enclosed OB associations and H I ridges have been correlated. Spherical, or more probably, cylindrical, neutral and ionized shells are proposed to explain these phenomena.

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