The authors concentrate their study of supernovae and supernova remnants on those areas
that are the newest, those in which the most unusual results have been obtained, and those …

Stellar Physics is a rather unique book among the growing literature on star formation and
evolution. Not only does the author, a leading expert in the field, give a very thorough …

Long-term monitoring of the radio emission from supernovae with the Very Large Array
(VLA) shows that the radio" light curves" evolve in a systematic fashion with a distinct peak …

The highly inclined spiral galaxy NGC 4258 (M106) has been observed in X-rays with the
PSPC of the Roentgen observatory ROSAT. Following X-ray components have been …

MERLIN observations at frequencies of 408, 1666 and 4995 MHz reveal 18 compact (< 0.25
arcsec) radio sources within the central few hundred parsecs of M82. M82 is well known as …

Based on the results of VLA observations, we report the detection of two unresolved radio
sources that are coincident with the reported optical position of SN 1923A in M83. For the …

Spatial, spectral, and timing analysis of deep ROSAT HRI and PSPC observations of the
active spiral galaxy NGC 4258 are reported. The diffuse emission of NGC 4258 has a 0.1 …

Some exploding stars (supernovae) are powerful emitters of centimeter radio radiation.
Detailed observations have shown that these supernovae quickly become detectable in the …

As part of an ongoing radio supernova monitoring program, we have discovered a variable,
compact steep spectrum radio source∼ 65 arcsec (∼ 4 kpc) from the centre of the starburst …

A study of the distribution of OH gas in the central region of the nearby active starburst
galaxy M82 has confirmed two previously known bright maser spots and revealed several …