Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..763g&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Nov.-Dec. 1980, p. 763-767.) Soviet Astronomy Letters, vol. 6, Nov.-Dec. 1980, p. 40
Astronomy and Astrophysics
Astronomy
1
Absorption Spectra, Formaldehyde, Interstellar Matter, Molecular Absorption, Optical Thickness, Radial Velocity, Radiative Recombination, Radio Astronomy
Scientific paper
Measurements of the 6.2-cm absorption line of the formaldehyde (H2CO) molecule have been obtained with a radio telescope having a resolution of 0.8 x 12 arcmin. The distribution of H2CO optical depth over the radio source Sgr B2 indicates that a gas envelope 11 pc in diameter may be present with a mean radial velocity close to the recombination-line velocities. The envelope is contracting at a rate of 20-25 km/sec and rotating at a peripheral velocity of 15 km/sec. The contraction in the central part of the molecular cloud surrounding Sgr B2 implies that it has a very short lifetime: roughly 5 x 10 to the 5th yr for matter in free fall.
Egorova T. M.
Gosachinskij I. V.
Grachev V. G.
Ivin G. N.
Komar N. P.
No associations
LandOfFree
Interstellar formaldehyde in Sagittarius B2 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 Interstellar formaldehyde in Sagittarius B2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interstellar formaldehyde in Sagittarius B2 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-757902