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| Content Provider | Springer Nature Link |
|---|---|
| Author | Ishida, Manabu |
| Copyright Year | 2010 |
| Abstract | The advent of the grating spectrometers onboard Chandra and XMM-Newton opened up a new era in plasma diagnostics of compact binaries. High resolution spectroscopy using these spectrometers is of particular use in investigating accretion plasmas in cataclysmic variables (CVs) because they show a wealth of emission lines owing to their optically thin thermal nature. In this review, I present recent progress on density measurements of the plasma in magnetic CVs by means of He-like triplet and iron L lines, and the outcome of line velocity measurements in the dwarf nova SS Cygni in outburst, to demonstrate the potential power of high resolution spectroscopy to elucidate the geometry of the plasma. In the end, our expectations for the Soft X-ray Spectrometer onboard the forthcoming X-ray mission Astro-H are summarized. |
| Starting Page | 155 |
| Ending Page | 165 |
| Page Count | 11 |
| File Format | |
| ISSN | 00386308 |
| Journal | Space Science Reviews |
| Volume Number | 157 |
| Issue Number | 1-4 |
| e-ISSN | 15729672 |
| Language | English |
| Publisher | Springer Netherlands |
| Publisher Date | 2010-12-11 |
| Publisher Place | Dordrecht |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Cataclysmic variables Plasma diagnostics He-like triplet Planetology Aerospace Technology and Astronautics Extraterrestrial Physics, Space Sciences Astrophysics and Astroparticles |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
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