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Elulookirjeldus (CV) | ||
1. | Eesnimi | Tiit |
2. | Perekonnanimi | Nugis |
3. | Töökoht | Tartu Observatoorium |
4. | Ametikoht | vanemteadur |
5. | Sünniaeg | 03.12.1942 (päev.kuu.aasta) |
6. | Haridus | TÜ (1969), optika-spektroskoopia |
7. | Teenistuskäik | Tartu Observatoorium (end. nimega Eesti TA AAI) - 1969 - 1977 nooremteadur; 1977 - 1990 vanemteadur; 1990 - k.a. juhtivteadur (vanemteadur) |
8. | Teaduskraad | füüs.-mat. kand. |
9. | Teaduskraadi välja andnud asutus, aasta |
TÜ, 1974 |
10. | Tunnustused | |
11. | Teadusorganisatsiooniline ja –administratiivne tegevus |
IAU ja EAS liige |
12. | Juhendamisel kaitstud väitekirjad |
Kalju Annuk, cand, 1990, juh. Tiit Nugis. Pikaperioodiliste Wolf-Rayet kaksiktätede uurimine. TÜ |
13. | Teadustöö põhisuunad | Astrofüüsika, kuumad suure absoluutheledusegs tähed, tähespektroskoopia, Wolf-Rayet tüüpi tähed, aine väljavool tähtedest ETFETF grant nr. |
14. | Jooksvad grandid | ETF grant nr. 6102 (grandihoidja), ETF grant nr. 5102 (põhitäitja) |
15. | Teaduspublikatsioonid |
Niedzielski A., Nugis T. and Skorzynski W. 2004. Kinematical structure of Wolf-Rayet winds. II. Internal scatter in WN stars. Acta Astronomica 54, 405-427 Niedzielski A., Nugis T. 2003. Hydrogen-to-helium ratio in WR stars from GAIA spectroscopy. In: GAIA Spectroscopy, Science and Technology. ASP Conf. Series Vol. 298, eds. U. Munari et al., 439-442 Lamers H.J.G.M. and Nugis T. 2002. An explanation for the curious mass loss history of massive stars: from OB stars, through Luminous Blue Variables to Wolf-Rayet stars. Astronomy & Astrophysics 395, L1-L5 Nugis T, and H.J.G.L.M. Lamers 2002. The mass-loss rates of Wolf-Rayet stars explained by optically thick radiation driven wind models. Astronomy & Astrophysics 389, 162-179 Nugis T. and H.J.G.L.M. Lamers 2000. Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters. Astronomy & Astrophysics 360, 227-244 Nugis T., Crowther P.A. and Willis A.J. 1998. Observations and analysis of the SVI 1975, 1993 lines in the IUE ultraviolet spectra of WN stars. Astronomy & Astrophysics 333, 956-968 |
viimati muudetud: 14.08.2005
Curriculum Vitae (CV) | ||
1. | First Name | Tiit |
2. | Surname | Nugis |
3. | Institution | Tartu Observatory |
4. | Position | senior research associate |
5. | Date of birth | 03.12.1942 (day.month.year) |
6. | Education | Tartu University (1969), optician-spectroscopist |
7. | Research and professional experience |
Tartu Observatory - 1969 - 1977 juniorresearch associate; 1977 - up to the present time senior research accociate |
8. | Academic degree | PhD |
9. | Dates and sites of earning the degrees |
TO, 1974 |
10. | Honours/awards | |
11. | Research-administrative experience |
the member of IAU and EAS |
12. | Supervised dissertations |
Kalju Annuk, cand, 1990, superv. Tiit Nugis. Pikaperioodiliste Wolf-Rayet kaksiktätede uurimine. TÜ |
13. | Current research program | Astrophysics, hot luminous stars, stellar spectroscopy, Wolf-Rayet stars, mass loss from stars |
14. | Current grant funding | ESF grant No. 6102 (grant-holder), ESF grant No. 5102 |
15. | List of most important publications |
Niedzielski A., Nugis T. and Skorzynski W. 2004. Kinematical structure of Wolf-Rayet winds. II. Internal scatter in WN stars. Acta Astronomica 54, 405-427 Niedzielski A., Nugis T. 2003. Hydrogen-to-helium ratio in WR stars from GAIA spectroscopy. In: GAIA Spectroscopy, Science and Technology. ASP Conf. Series Vol. 298, eds. U. Munari et al., 439-442 Lamers H.J.G.M. and Nugis T. 2002. An explanation for the curious mass loss history of massive stars: from OB stars, through Luminous Blue Variables to Wolf-Rayet stars. Astronomy & Astrophysics 395, L1-L5 Nugis T, and H.J.G.L.M. Lamers 2002. The mass-loss rates of Wolf-Rayet stars explained by optically thick radiation driven wind models. Astronomy & Astrophysics 389, 162-179 Nugis T. and H.J.G.L.M. Lamers 2000. Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters. Astronomy & Astrophysics 360, 227-244 Nugis T., Crowther P.A. and Willis A.J. 1998. Observations and analysis of the SVI 1975, 1993 lines in the IUE ultraviolet spectra of WN stars. Astronomy & Astrophysics 333, 956-968 |
last updated: 14.08.2005
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