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The Growth, Polarization, and Motion of the Radio Afterglow from the Giant Flare from SGR 1806-20

(2005)

Authors:

GB Taylor, JD Gelfand, BM Gaensler, J Granot, C Kouveliotou, RP Fender, E Ramirez-Ruiz, D Eichler, YE Lyubarsky, M Garrett, RAMJ Wijers
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Rapid variability of the arcsec-scale X-ray jets of SS 433

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 358:3 (2005) 860-868

Authors:

S Migliari, RP Fender, KM Blundell, M Mendez, M Van Der Klis
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Energisation of interstellar media and cosmic ray production by jets from X-ray binaries

(2005)

Authors:

Rob Fender, Tom Maccarone, Zdenko van Kesteren
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POINT-AGAPE Pixel Lensing Survey of M31 : Evidence for a MACHO contribution to Galactic Halos

(2005)

Authors:

S Calchi Novati, S Paulin-Henriksson, J An, P Baillon, V Belokurov, BJ Carr, M Creze, NW Evans, Y Giraud-Heraud, A Gould, P Hewett, Ph Jetzer, J Kaplan, E Kerins, SJ Smartt, CS Stalin, Y Tsapras, MJ Weston
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Hot Cores : Probes of High-Redshift Galaxies

ArXiv astro-ph/0504040 (2005)

Authors:

CJ Lintott, S Viti, DA Williams, JMC Rawlings, I Ferreras

Abstract:

The very high rates of second generation star formation detected and inferred in high redshift objects should be accompanied by intense millimetre-wave emission from hot core molecules. We calculate the molecular abundances likely to arise in hot cores associated with massive star formation at high redshift, using several independent models of metallicity in the early Universe. If the number of hot cores exceeds that in the Milky Way Galaxy by a factor of at least one thousand, then a wide range of molecules in high redshift hot cores should have detectable emission. It should be possible to distinguish between independent models for the production of metals and hence hot core molecules should be useful probes of star formation at high redshift.
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