| Proposal ID | 082023 |
| Title | Do X-rays Make Disk Emission Lines in Quiescent Dwarf Novae? |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0820230101 |
| DOI | https://doi.org/10.5270/esa-hwe1ky1 |
| Principal Investigator, PI | Dr Knox Long |
| Abstract | If the standard disk instability model for outbursts in dwarf novae (DNe) iscorrect, the disk in quiescence should be cold and optically thick. Butquiescent DNe show UV and optical emission lines. Why? Is the disk opticallythin in the continuum? Does viscous dissipation near the disk photosphereproduce a corona? Or, is a corona created by X-ray illumination of the disk froma hot boundary layer? Here we propose to test the X-ray illumination hypothesiswith simultaneous, highly time-resolved observations of SS Cyg in quiescencewith XMM-Newton and HST/STIS. The X-ray flux in SS Cyg varies on shorttimescales. If X-ray illumination is responsible for the emission lines, theyshould vary in response to the X-ray flux. If not, one of the other mechanisms must be responsible. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2018-11-24T07:23:42Z/2018-11-24T23:52:02Z |
| Version | 19.17_20220121_1250 |
| Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis. |
| Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
| Date Published | 2019-12-19T23:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "time resolved", "disk photosphere", "xmm newton", "quiescent dne", "ss cyg", "disk emission lines", "xray illumination", "optical emission lines", "hot boundary layer", "corona created", "viscous dissipation", "emission lines", "XMM-Newton", "xray flux", "HST", "optically thick", "dwarf novae dne", "ss cyg varies", "XMM", "disk optically thin", "xray illumination hypothesis", "short timescales" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Knox Long, 2019, 'Do X-rays Make Disk Emission Lines in Quiescent Dwarf Novae?', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-hwe1ky1 |