On the structure of M17S

Details On the structure of M17S On the structure of M17S

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf...49a&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 49-51 (SEE

Physics

Cosmic Dust, Galactic Structure, Near Infrared Radiation, Nebulae, Particle Density (Concentration), Photons, Radiation Sources, Spectral Bands, Ultraviolet Radiation

Scientific paper

The behavior of the 9.7 micron band due to dust particles was studied
for some positions within M17S. This source is probably
ultraviolet-photon-bounded, with cool dust in front.

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