RX J0152.7−1357: Stellar Populations in an X-Ray Luminous Galaxy Cluster at z = 0.83
The Astronomical Journal American Astronomical Society 129:3 (2005) 1249-1286
The discovery of a type II quasar at z= 1.65 with integral-field spectroscopy
\mnras 358 (2005) L11-L15-L11-L15
An expanding radio nebula produced by a giant flare from the magnetar SGR 1806-20
(2005)
Molecular abundance ratios as a tracer of accelerated collapse in regions of high-mass star formation
Astrophysical Journal 620:2 I (2005) 795-799
Abstract:
Recent observations suggest that the behavior of tracer species such as N2H+ and CS is significantly different in regions of high- and low-mass star formation. In the latter, N2H+ is a good tracer of mass, while CS is not. Observations show the reverse to be true in high-mass star formation regions. We use a computational chemical model to show that the abundances of these and other species may be significantly altered by a period of accelerated collapse in high-mass star-forming regions. We suggest that these results provide a potential explanation of the observations, and make predictions for the behavior of other species. © 2005. The American Astronomical Society. All rights reserved.The POINT-AGAPE survey — II. An unrestricted search for microlensing events towards M31
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 357:1 (2005) 17-37