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New Estimates of the Solar-Neighborhood Massive Star Birthrate and the Galactic Supernova Rate The birthrate of stars of masses >=10 Msolar is estimatedfrom a sample of just over 400 O3-B2 dwarfs within 1.5 kpc of the Sunand the result extrapolated to estimate the Galactic supernova ratecontributed by such stars. The solar-neighborhood Galactic-plane massivestar birthrate is estimated at ~176 stars kpc-3Myr-1. On the basis of a model in which the Galactic stellardensity distribution comprises a ``disk+central hole'' like that of thedust infrared emission (as proposed by Drimmel and Spergel), theGalactic supernova rate is estimated at probably not less than ~1 normore than ~2 per century and the number of O3-B2 dwarfs within the solarcircle at ~200,000.
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| Spectral classification of ultraviolet objects. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1978A&A....66L...9B&db_key=AST
| Luminous stars in a region south of h and chi Persei. With 3 Figures in the Text Not Available
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Osservazione e dati astrometrici
Costellazione: | Andromeda |
Ascensione retta: | 23h52m48.77s |
Declinazione: | +46°28'22.7" |
Magnitudine apparente: | 9.495 |
Moto proprio RA: | -6.5 |
Moto proprio Dec: | -1 |
B-T magnitude: | 9.313 |
V-T magnitude: | 9.48 |
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