Olesya Vladimirovna Kozlova |
||||
birthdate: | May 12, 1969 |
Address |
||
birthplace: | Orsha city, Belorussia | Crimean Astrophysical Observatory 298409, Nauchny Crimea Russia |
||
phone: | +7 (36554) 71507 | |||
fax: | +7 (36554) 71004 | |||
e-mail: | oles_kozlova @mail.ru | |||
Academic Degrees
1991 | M.Sc. (Astronomy) Leningrad State University, Russia |
2005 | Ph.D. (Astrophysics) Pulkovo, St-Peterburg, Russia |
Principal Employment:
1991-1994 | Post-graduated student |
1994-2003 | Junior research scientist, Crimean Astrophysical Observatory (CrAO) |
2003-present | Scientist, CrAO |
Theses:
Degree | Title | Advisor |
---|---|---|
M. Sc. | The modeling of synthetic spectra of Mira type stars | S.V. Berduygina |
Ph. D. | Spectral variability of UX Ori type stars | V.P. Grinin |
Research Interests:
Yong stars with non-periodic Algol-type minima, UX Ori type stars, Ae/Be Herbig stars, protoplanetary disks, accretion disks, disk wind
Participation in Projects:
Stars on early stages of evolution (Evolution)
Selected publications:
- Kozlova O.V., Grinin V.P., Rostopchina A.N. - УSpectroscopic evidence of sporadic gas accretion onto the Herbig Ae stars with non-periodic Algol-type minimaУ - Astron. and Astrophys. Transactions, 1995, V.8, P.249-259.
- Grinin V.P., Kozlova O.V., The P.S., Rostopchina A.N. - "The ? Pictoris phenomenon among young stars. III. The Herbig Ae stars WW Vulpeculae, RR Tauris and BF Orionis" - Astron. Astrophys., 1996, V.309, P.474-480.
- Kozlova O.V., Grinin V.G., Rostopchina A.N. - "Non-Stationary Gas Accretion on UX Ori type stars" - Astron. Astrophys. Transaction, 1998, V.15, P.153-157.
- Beskrovnaya N.G., Pogodin M.A., Mirpshnichenko A.S., The P.S., Savanov I.S., Shakhovskoy N.M., Rostopchina A.N., Kozlova O.V., Kuratov K.S. - ТSpectroscopic, photometric, and polarimetric study of the Herbig Ae candidate HD 361У, Astron. and Astrophys., 1999, V.343, P.163.
- Grinin V.P., Kozlova O.V., Natta A., Ilyin I., Touminen I., Rostopchina A.N. - "Optical spectra of five UX Ori-type stars" Р Astron. Astrophys., 2001, V.379, P.482-495.