The coherence of radiation by fast-moving charges

Details The coherence of radiation by fast-moving charges The coherence of radiation by fast-moving charges

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..117k&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 1, Sept. 1980, p. 117-125.

Astronomy and Astrophysics

Astrophysics

Coherent Radiation, Neutron Stars, Stellar Radiation, Cubic Lattices, Galactic Bulge, Wavelengths

Scientific paper

It is shown that the 2.6 mm CO emission profile in the regions of two unidentified 2.4-micron features (at l = 356 deg and l = 5 deg) near the galactic center is consistent with an explanation of these features in terms of inhomogeneities in interstellar extinction. The mass-to-luminosity ratio of the galactic central bulge is estimated to be M/L(v) = 4.

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