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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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