Structural details of the Orion Nebula - Detection of a network of stringlike ionized features

Details Structural details of the Orion Nebula - Detection of a network of stringlike ionized features Structural details of the Orion Nebula - Detection of a network of stringlike ionized features

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...361l..19y&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 361, Sept. 20, 1990, p. L19-L22. Research supported by the Northw

Astronomy and Astrophysics

Astrophysics

41

H Ii Regions, Orion Nebula, Interstellar Gas, Very Large Array (Vla)

Scientific paper

Continuum observations of the Orion Nebula, obtained at 20 cm using the A, B, C, and D configurations of the VLA during 1986-1987, are reported. Radio images of resolution 1.8 x 1.6 arcsec are presented and analyzed, with a focus on (1) the complex cone structure of M 42 and (2) an extended network of bright stringlike features concentrated near the Trapezium cluster. Possible theoretical explanations of these features are explored, starting from the blister model of H II regions developed by Tenorio and Tagle (1979).

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