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E. Gonzalez, D. Pooley, W. Lewin (MIT)
We present results of five Chandra observations (of ~20 ksec each) spaced over 20 months of the normal galaxy NGC 3877. Our analysis of a roughly 6 by 6 arcmin region around the galaxy reveals 48 sources, many of which are likely background objects. We provide lightcurves, hardness ratios, and luminosity estimates for each source and discuss the X-ray source population of the galaxy.
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.