Rubin-LSST

Research group

Research theme

Sub department

About

The discovery of a type II quasar at ɀ = 1.65 with integral-field spectroscopy

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 358:1 (2005) l11-l15

Authors:

Matt J Jarvis, Caroline van Breukelen, RJ Wilman
More details from the publisher
More details

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

Authors:

Inger Jørgensen, Marcel Bergmann, Roger Davies, Jordi Barr, Marianne Takamiya, David Crampton
More details from the publisher
More details
Details from ArXiV

The discovery of a type II quasar at z= 1.65 with integral-field spectroscopy

\mnras 358 (2005) L11-L15-L11-L15

Authors:

MJ Jarvis, C van Breukelen, RJ Wilman
More details from the publisher
More details
Details from ArXiV

An expanding radio nebula produced by a giant flare from the magnetar SGR 1806-20

(2005)

Authors:

BM Gaensler, C Kouveliotou, JD Gelfand, GB Taylor, D Eichler, RAMJ Wijers, J Granot, E Ramirez-Ruiz, YE Lyubarsky, RW Hunstead, D Campbell-Wilson, AJ van der Host, MA McLaughlin, RP Fender, MA Garrett, KJ Newton-McGee, DM Palmer, N Gehrels, PM Woods
More details from the publisher

Molecular abundance ratios as a tracer of accelerated collapse in regions of high-mass star formation

Astrophysical Journal 620:2 I (2005) 795-799

Authors:

CJ Lintott, S Viti, JMC Rawlings, DA Williams, TW Hartquist, P Caselli, I Zinchenko, P Myers

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.
More details from the publisher