ar X iv : a st ro - p h / 96 01 16 3 v 1 2 9 Ja n 19 96 Lagrangian Dynamics of Collisionless Matter

ar X iv : a st ro - p h / 96 01 12 9 v 1 2 3 Ja n 19 96 Is Her X - 1 a strange star

The possible identification of Her X-1 with a strange star (Li et al. 1995) is shown to be incorrect.

ar X iv : a st ro - p h / 97 01 22 8 v 1 2 9 Ja n 19 97 Large - scale Structures revealed by Wavelet Decomposition 1

ar X iv : a st ro - p h / 96 06 17 9 v 1 2 9 Ju n 19 96 LECTURE 1 Coalescence of Binary Neutron Stars

ar X iv : a st ro - p h / 96 01 19 1 v 1 3 1 Ja n 19 96 NGC 2915 . II . A Dark Spiral Galaxy With A Blue Compact Dwarf Core

This paper presents Australia Telescope Compact Array H I synthesis observations of the weak blue compact dwarf (BCD) galaxy NGC 2915. It is shown that NGC 2915 has the H I properties of a late type spiral galaxy (Sd Sm), including a double horn global profile, and H I spiral arms. The H I extends out to over five times the Holmberg radius, and 22 times the exponential scale length in the B ban...

ar X iv : a st ro - p h / 96 01 16 7 v 1 2 9 Ja n 19 96 BATSE SD Observations of Hercules X - 1

The cyclotron line in the spectrum of the accretion-powered pulsar Her X-1 offers an opportunity to assess the ability of the BATSE Spectroscopy Detectors (SDs) to detect lines like those seen in some GRBs. Preliminary analysis of an initial SD pulsar mode observation of Her X-1 indicated a cyclotron line at an energy of ≈ 44 keV, rather than at the expected energy of ≈ 36 keV. Our analysis of ...