Hα Observations of the Rosette Nebula and the Distribution of Interstellar Dust

Details Hα Observations of the Rosette Nebula and the Distribution of Interstellar Dust Hα Observations of the Rosette Nebula and the Distribution of Interstellar Dust

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983msngr..32...23c&link_type=abstract

The Messenger, No. 32:JUN, P.23, 1983

Physics

7

Scientific paper

The Rosette nebula is a well-known HII region in the constellation of Monoceros with a diameter of more than 2°. The nebula has a nearly circular shape forming a ring around a deep local intensity minimum (Fig. 1). The open star cluster NGC 2244 is visible within the HI1 region, containing early-type stars which emit enough hard UV radiation to ionize the nebula. Adjacent to the north-eastern border of the Rosette nebula there is the large supernova remnant of the Monoceros Loop.

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