On the origin of tightly wound spiral features in galactic nuclei

Details On the origin of tightly wound spiral features in galactic nuclei On the origin of tightly wound spiral features in galactic nuclei

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....20....7p&link_type=abstract

(Astrofizika, vol. 20, Jan.-Feb. 1984, p. 7-20) Astrophysics (ISSN 0571-7132), vol. 20, no. 1, July 1984, p. 1-10. Translation.

Astronomy and Astrophysics

Astrophysics

5

Galactic Nuclei, Galactic Structure, Rotating Matter, Spiral Galaxies, Astronomical Models, Astronomical Spectroscopy

Scientific paper

A mechanism for the origin and development of spiral arms proposed earlier by one of the authors (P. P.) is recalled to show that spiral structure in the nucleus of a galaxy can be produced by matter ejected from a rotating nucleus. The mechanism can account for the observations of outward and/or inward motions in the nuclear regions of spirals. In particular the model applied to the tight nuclear spiral of NGC 4736 shows satisfactory agreement with observations.

Affiliated with

Also associated with

No associations

Rating

On the origin of tightly wound spiral features in galactic nuclei 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 On the origin of tightly wound spiral features in galactic nuclei, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the origin of tightly wound spiral features in galactic nuclei will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-935247