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Post Info TOPIC: SU Ursae Majoris


L

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RE: SU Ursae Majoris
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The dwarf nova SU UMa is in outburst.

Date: 30th March, 2011
Magnitude range: 10.8 - 14.96 V
Period: 19 days
Satellite period: 0.07635 days
Type: UGSU

Position(2000): RA=08 12 28.26, Dec=+62° 36' 22.5"



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Title: X-ray observations of SU UMa throughout six outbursts
Authors: David J. Collins, Peter J. Wheatley

We present RXTE observations covering six normal outbursts of the dwarf nova SU UMa, the prototype of its class. The outbursts showed consistent X-ray behaviour with the X-ray count rate dropping suddenly by a factor of our, and with evidence for a half day delay between the optical rise and the X-ray suppression. In contrast to SS Cyg, an X-ray flux increase at the beginning of outburst was not observed, although it is expected from boundary layer models. The X-ray flux was high and decreasing during quiescence, in conflict with the disc instability model. The X-ray spectrum of SU UMa was softer in outburst than during quiescence, and it was consistent with constant reflection.

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-- Edited by Blobrana on Wednesday 18th of November 2009 05:38:47 PM

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There are three subtypes of U Geminorum star (UG):

  1. SS Cygni stars (UGSS), which increase in brightness by 2-6 mag in V in 1-2 days, and return to their original brightnesses in several subsequent days.
  2. SU Ursae Majoris stars (UGSU), which have brighter and longer "supermaxima" outbursts, or "super-outbursts," in addition to normal outbursts. Varieties of SU Ursae Majoris star include ER Ursae Majoris stars and WZ Sagittae stars.
  3. Z Camelopardalis stars (UGZ), which temporarily "halt" at a particular brightness below their peak.

Source



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