Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...137..223c&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 137, no. 2, Aug. 1984, p. 223-234.
Astronomy and Astrophysics
Astronomy
17
Binary Stars, Galactic Nuclei, Local Group (Astronomy), Radio Stars, Stellar Spectra, X Ray Sources, Stellar Evolution, Stellar Models, Ultraviolet Astronomy, X Ray Stars
Scientific paper
The λλ1200 - 3000 Å spectrum of the nucleus of M33 is used in conjunction with U, B, V photometry as input to a linear programming method to determine the stellar population of the system. No astrophysical constraints but modifications in the stellar library (which includes Population II objects) were used to explore different evolutionary histories of star formation in the nucleus. A multigeneration model, where a young component (age ≡107years) and an old one (age ≡5×109 years) are superimposed, gives the best fit to the data and is favoured by the results at other wavelengths as well. The effect of reddening on the modelling and the interpretation of the nuclear X-ray source are briefly discussed.
Benvenuti Piero
Ciani Antonia
Dodorico Sandro
No associations
LandOfFree
The stellar population of the nucleus of M 33 from an analysis of its 1200-3000 A spectrum 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 The stellar population of the nucleus of M 33 from an analysis of its 1200-3000 A spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The stellar population of the nucleus of M 33 from an analysis of its 1200-3000 A spectrum will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1673544