Observations of the atoms in highly excited states, close to the limit in the Galaxy

Details Observations of the atoms in highly excited states, close to the limit in the Galaxy Observations of the atoms in highly excited states, close to the limit in the Galaxy

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..396l&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, May 1989, p. 396-399. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Atomic Excitations, Milky Way Galaxy, Radio Astronomy, Absorption Spectra, Bohr Theory, Line Spectra, Orbit Calculation

Scientific paper

The recombination radiolines C593-alpha and C747-beta have been detected
at a frequency of 31.4 MHz in absorption towards Cas A. The C747-beta
line corresponds to the highest observed atomic excitation level. The
dimension of the Bohr orbits of the atom at this excitation level is
about 0.06 mm, near the limit in the Galaxy.

Affiliated with

Also associated with

No associations

Rating

Observations of the atoms in highly excited states, close to the limit in the Galaxy 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 Observations of the atoms in highly excited states, close to the limit in the Galaxy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of the atoms in highly excited states, close to the limit in the Galaxy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1875231