Astrophysics of red supergiants /
Astrophysics of Red Supergiants' is the first book of its kind devoted to our current knowledge of red supergiant stars, a key evolutionary phase that is critical to our larger understanding of massive stars. It provides a comprehensive overview of the fundamental physical properties of red sup...
| Κύριος συγγραφέας: | |
|---|---|
| Μορφή: | Ηλ. βιβλίο |
| Γλώσσα: | English |
| Έκδοση: |
Bristol :
IOP Publishing,
c2017.
|
| Σειρά: | IOP astronomy.
AAS-IOP Astronomy. |
| Θέματα: | |
| Διαθέσιμο Online: | https://iopscience.iop.org/book/978-0-7503-1329-2 |
| LEADER | 03579nam a2200445 i 4500 | ||
|---|---|---|---|
| 001 | 9780750313292 | ||
| 003 | IOP | ||
| 005 | 20190321140751.0 | ||
| 006 | m eo d | ||
| 007 | cr cn |||m|||a | ||
| 008 | 180111s2017 enka ob 000 0 eng d | ||
| 999 | |c 140236 |d 140236 | ||
| 020 | |a 9780750313292 |q ebook | ||
| 020 | |a 9780750313315 |q mobi | ||
| 020 | |z 9780750313308 |q print | ||
| 040 | |a CaBNVSL |b gre |e AACR2 |c GR-PaULI |d GR-PaULI | ||
| 082 | 0 | 4 | |a 523.8 |2 23 |
| 100 | |a Levesque, Emily M. |e συγγραφέας. |9 174718 | ||
| 245 | 1 | 0 | |a Astrophysics of red supergiants / |c Emily M. Levesque. |
| 260 | |a Bristol : |b IOP Publishing, |c c2017. | ||
| 300 | |a 1 ηλεκτρονική πηγή (ποικίλες σελιδαριθμήσεις) : |b εικ. (μερ. έγχρ.). | ||
| 490 | 1 | |a AAS-IOP Astronomy | |
| 490 | 1 | |a IOP astronomy, |x 2514-3433 | |
| 504 | |a Περιλαμβάνει βιβλιογραφικές παραπομπές. | ||
| 505 | 0 | |a 1. An introduction to red supergiants -- 1.1. A key evolutionary phase -- 1.2. Supernova progenitors -- 1.3. Extragalactic probes | |
| 505 | 8 | |a 2. Inside a red supergiant -- 2.1. Evolution and the stellar core -- 2.2. Envelopes and atmospheres | |
| 505 | 8 | |a 3. Physical properties of red supergiants -- 3.1. The spectrum of a red supergiant -- 3.2. Effective temperatures -- 3.3. Masses -- 3.4. Luminosities -- 3.5. Radii -- 3.6. Surface gravities | |
| 505 | 8 | |a 4. Mass loss and dust production in red supergiants -- 4.1. Winds and mass-loss processes -- 4.2. Dust from supergiants -- 4.3. Extreme Mass Loss in RSGs--OH/IR supergiants | |
| 505 | 8 | |a 5. Red supergiants in binaries -- 5.1. Modeling RSG binaries -- 5.2. Observing RSGs in binaries : the VV Cep and [Zeta] Aur systems -- 5.3. Extreme binary scenarios for RSGs | |
| 505 | 8 | |a 6. Red supergiants in and beyond the Milky Way -- 6.1. Identifying red supergiant populations -- 6.2. RSGs in the Milky Way -- 6.3. Extragalactic RSG populations -- 6.4. Metallicity effects in rsgs | |
| 505 | 8 | |a 7. Variability in red supergiants -- 7.1. Photometric variability -- 7.2. Spectroscopic variability | |
| 505 | 8 | |a 8. Red supergiants and supernovae -- 8.1. RSGs as direct progenitors--Type II-P supernovae -- 8.2. The "red supergiant problem" -- 8.3. RSGs as progenitor precursors | |
| 505 | 8 | |a 9. The future of red supergiant research -- 9.1. Time domain astronomy -- 9.2. Beyond the local group -- 9.3. NGC 6946 : an example of RSG astronomy in the 2020s. | |
| 520 | 3 | |a Astrophysics of Red Supergiants' is the first book of its kind devoted to our current knowledge of red supergiant stars, a key evolutionary phase that is critical to our larger understanding of massive stars. It provides a comprehensive overview of the fundamental physical properties of red supergiants, their evolution, and their extragalactic and cosmological applications. It serves as a reference for researchers from a broad range of fields (including stellar astrophysics, supernovae, and high-redshift galaxies) who are interested in red supergiants as extreme stages of stellar evolution, dust producers, supernova progenitors, extragalactic metallicity indicators, members of massive binaries and mergers, or simply as compelling objects in their own right. The book is accessible to a range of experience levels, from graduate students up to senior researchers. | |
| 650 | 0 | |a Άστρα |9 4291 | |
| 650 | 0 | |a Αστροφυσική |9 125 | |
| 830 | 0 | |a IOP astronomy. | |
| 830 | 0 | |a AAS-IOP Astronomy. | |
| 856 | 4 | 0 | |u https://iopscience.iop.org/book/978-0-7503-1329-2 |
| 942 | |2 ddc |c ERS | ||
