HST Spectroscopy of the Nucleus of M33

Details HST Spectroscopy of the Nucleus of M33 HST Spectroscopy of the Nucleus of M33

2001-12-13

arxiv.org/abs/astro-ph/0112327v1

Astronomy and Astrophysics

Astrophysics

24 pages, including 6 figures. accepted for publication in ApJ, v569 (April 10, 2002)

Scientific paper

We have used Hubble Space Telescope to obtain moderate resolution 1150-5700 Ang. spectroscopy of the nucleus of M33 and a blue star ~1 arcsec NNW of the nucleus in an attempt to find the optical counterpart of the nuclear X-ray source and to characterize stellar populations in the nuclear region. The STIS spectra of the nucleus can be modelled in terms of two starbursts, one with a mass of about 9000 solar masses at 40 Myrs and the other with a mass of about 76,000 solar masses at 1 Gyrs. The blue star is a late type O giant, with no obvious spectral anomalies to indicate that it is associated with the luminous X-ray source. The nuclear region is not heavily reddened; 2200 Ang absorption features in the spectra of both the nucleus and the star are weak. The data and the star formation history support the hypothesis that the M33 nuclear source, the brightest persistent source in the Local group, is an ~10 solar mass black hole binary.

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