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IMBH formation • if an IMBH, cannot form from evolution of high metallicity stars ...
IMBH formation • if an IMBH, cannot form from evolution of high metallicity stars ... • three merging scenarios
Page 1 and 2: Optical studies of an ultraluminous
Page 3 and 4: ultraluminous X-ray sources
Page 5 and 6: ultraluminous X-ray sources • ULX
Page 7 and 8: ultraluminous X-ray sources • ULX
Page 9 and 10: ULXs in NGC1313 • a barred SB(s)d
Page 11 and 12: X-ray observations: light curves Za
Page 13 and 14: X-ray observations: spectroscopy
Page 15 and 16: optical observations ESO 3.6m R cou
Page 17 and 18: optical observations
Page 19 and 20: optical observations: astrometry
Page 21 and 22: optical observations: astrometry x3
Page 23 and 24: optical observations: astrometry
Page 25 and 26: optical observations: environments
Page 27 and 28: optical observations: photometry
Page 29 and 30: optical observations: variability
Page 31 and 32: color-magnitude diagrams • two po
Page 33 and 34: spectral energy distribution
Page 35 and 36: spectral energy distribution
Page 37: IMBH formation
Page 41 and 42: IMBH formation • if an IMBH, cann
Page 43 and 44: adial velocity
Page 45 and 46: adial velocity Pakull et al. 2006 H
Page 47 and 48: adial velocity • if He II line fr
Page 49 and 50: adial velocity • if He II line fr
Page 51: adial velocity • if He II line fr

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