Difference between revisions of "Triggers:DNe"
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* Example of a dwarf nova GK Perseii ([http://arxiv.org/abs/0907.1407 Evans et al. 2009]) : detection of an outburst led to Swift, UV and X-rays follow up. It revealed unusual outburst in the optical but typical outburst in X, challenging existing disc outburst models. | * Example of a dwarf nova GK Perseii ([http://arxiv.org/abs/0907.1407 Evans et al. 2009]) : detection of an outburst led to Swift, UV and X-rays follow up. It revealed unusual outburst in the optical but typical outburst in X, challenging existing disc outburst models. | ||
| − | [[File:GKPer.png| | + | [[File:GKPer.png|400px|thumb|left|AAVSO lightcurve of outbursts of dwarf nova GK Per since 1954]] |
Revision as of 17:48, 10 July 2009
Dwarf noave have relatively small amplitude outbursts repeating in timescales between days and many years.
- Example of a dwarf nova GK Perseii (Evans et al. 2009) : detection of an outburst led to Swift, UV and X-rays follow up. It revealed unusual outburst in the optical but typical outburst in X, challenging existing disc outburst models.
