Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...301..813o&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 301, Feb. 15, 1986, p. 813-824. Research supported by the University of Mar
Astronomy and Astrophysics
Astronomy
22
Astronomical Maps, Astronomical Spectroscopy, Decametric Waves, Nebulae, Radio Astronomy, Supernova Remnants, Absorption Spectra, Data Reduction, Electron Energy, Gas Temperature, H Ii Regions
Scientific paper
Observations are presented at 20.6, 25.6, and 30.9 MHz of a field containing the Rosette Nebula and the Monoceros Loop supernova remnant. From the maps presented here, it appears that radiation from the supernova remnant (SNR) is being absorbed by the Rosette Nebula, suggesting that the SNR is located behind the H II region but still within the Mon OB2 association, at a distance of ≡1.6 kpc. An electron temperature on the order of 8000K is obtained for the diffuse ionized gas in the Monoceros Loop, and it is suggested that this gas is photoionized by members of the Mon OB2 association. A mean electron temperature of 8700±1300K is derived for the Rosette Nebula.
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