2.4 micron emission from the galactic centre region

Details 2.4 micron emission from the galactic centre region 2.4 micron emission from the galactic centre region

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..111h&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 1, Sept. 1980, p. 111-116.

Astronomy and Astrophysics

Astronomy

2

Galactic Nuclei, Galactic Radiation, Infrared Astronomy, Milky Way Galaxy, Carbon Monoxide, Galactic Bulge, Isophotes, Luminosity

Scientific paper

It is shown that the 2.6 mm CO emission profile in the regions of two unidentified 2.4-micron features observed near the galactic center is consistent with an explanation of these features in terms of inhomogeneities in interstellar extinction. From the observations the mass to luminosity ratio of the galactic central bulge is estimated to be 4.

Affiliated with

Also associated with

No associations

Rating

2.4 micron emission from the galactic centre region does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with 2.4 micron emission from the galactic centre region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 2.4 micron emission from the galactic centre region will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-904049