Eric M. Schlegel

Chandra High-Resolution Camera observations of the luminous X-ray source in the starburst galaxy M82

We have analyzed Chandra High Resolution Camera observations of the starburst galaxy M82, concentrating on the most luminous x-ray source. We find a position for the source of

The Luminosity of SN 1999by in NGC 2841 and the Nature of “Peculiar” Type Ia Supernovae

\rm R.A. = 09^h 55^m 50^s.2, decl. = +69^{\circ} 40\arcmin 46\arcsec.7

NEW SPECTRAL CLASSIFICATION TECHNIQUE FOR X-RAY SOURCES: QUANTILE ANALYSIS

(J2000) with a

A DETERMINATION OF THE SPIN OF THE BLACK HOLE PRIMARY IN LMC X-1

1\sigma

X-Ray Processing of ChaMPlane Fields: Methods and Initial Results for Selected Anti-Galactic Center Fields

radial error of

An X-ray and optical study of the supernova remnant W44

0.7\arcsec

SN 1978K: An extraordinary supernova in the nearby galaxy NGC 1313

. The accurate x-ray position shows that the luminous source is not at the dynamical centre of M82 nor coincident with any suggested radio AGN candidate. The source is highly variable between observations, which suggests that the source is a compact object and not a supernova or remnant. There is no significant short term variability within the observations. Dynamical friction and the off-center position place an upper bound of

Chandra multiwavelength project. II. First results of X-ray source properties

10^{5} - 10^{6} M_{\odot}

Doppler imaging of the dwarf nova U Geminorum

on the mass of the object, depending on its age. The x-ray luminosity suggests a compact object mass of at least

X-ray emission from supernovae: a review of the observations

500 M_{\odot}