Browsing by Subject "library"

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    The Literature Review Survival Guide 2014
    (2014-08-25) d'Angelo, Alex
    This guide will help you to find full text electronic information for tutorials and essays.
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    Mistress Serendipity's Library
    (2014-08-28) d'Angelo, Alex
    Steer Mistress Serendipity on her broom to connect to top-quality free e-resources, useful for high schools and colleges. This game has been designed to help high-school and college students discover top-quality web resources in a fun and exciting way. To use this resource: download the zip file, Extract all in the zip file and click on 'HagLib' to launch the game. This resource was updated on 12 January 2015.
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    Open Access
    Radio monitoring of the hard state jets in the 2011 outburst of MAXI J1836−194
    (2015) Russell, T D; Miller-Jones, J C A; Curran, P A; Soria, R; Altamirano, D; Corbel, S; Coriat, M; Moin, A; Russell, D M; Sivakoff, G R; Slaven-Blair, T J; Belloni, T M; Fender, R P; Heinz, S; Jonker, P G; Krimm, H A; Körding, E G; Maitra, D; Markoff, S; Middleton, M; Migliari, S; Remillard, R A; Rupen, M P; Sarazin, C L; Tetarenko, A J; Torres, M A P; Tudose, V; Tzioumis, A K
    MAXI J1836-194 is a Galactic black hole candidate X-ray binary that was discovered in 2011 when it went into outburst. In this paper, we present the full radio monitoring of this system during its 'failed' outburst, in which the source did not complete a full set of state changes, only transitioning as far as the hard intermediate state. Observations with the Karl G. Jansky Very Large Array (VLA) and Australia Telescope Compact Array (ATCA) show that the jet properties changed significantly during the outburst. The VLA observations detected linearly polarised emission at a level of ~1% early in the outburst, increasing to ~3% as the outburst peaked. High-resolution images with the Very Long Baseline Array (VLBA) show a ~15 mas jet along the position angle -21 ± 2o, in agreement with the electric vector position angle found from our polarisation results (-21 ± 4o), implying that the magnetic field is perpendicular to the jet. Astrometric observations suggest that the system required an asymmetric natal kick to explain its observed space velocity. Comparing quasi-simultaneous X-ray monitoring with the 5 GHz VLA observations from the 2011 outburst shows an unusually steep hard-state radio/X-ray correlation of LR ∝ LX1.8±0.2, where LR and LX denote the radio and X-ray luminosities, respectively. With ATCA and Swift monitoring of the source during a period of re-brightening in 2012, we show that the system lay on the same steep correlation. Due to the low inclination of this system, we then investigate the possibility that the observed correlation may have been steepened by variable Doppler boosting.