Optical and near-IR study of LMC HII region N11AB

Details Optical and near-IR study of LMC HII region N11AB Optical and near-IR study of LMC HII region N11AB

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3084..157l&link_type=abstract

In NASA, Ames Research Center, The Interstellar Medium in External Galaxies: Summaries of Contributed Papers p 157-159 (SEE N91-

Computer Science

Cosmic Dust, Emission, H Ii Regions, Ionized Gases, Photometry, Star Clusters, Embedding, Near Infrared Radiation

Scientific paper

N11 (DEM 34), complex HII region located about 4 degrees from the center of the LMC bar, is a very interesting giant interstellar shell. It has a complicated structure and motion. It is located on the edge of an HI concentration. This is the progress report of the study of its two components, A and B at the optical and near-IR wavelengths to investigate stars, dust and ionized gas associated with them. N11A is a compact high-excitation blob and N11B is a bright HII region in this complex, which embeds OB association Lucke-Hodge 10.

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