List of published papers
Contact binaries and multiple systems
- Pribulla, T., Chochol, D., Rovithis, P., Rovithis-Livaniou, H.: 1997,
Sudden period change in the contact binary AW UMa, Inf. Bull.
Variable Stars, 4435
IBVS
- Pribulla, T., Chochol, D., Rovithis-Livaniou, H., Rovithis, P.: 1998,
Angular momentum loss in the multiple system AW UMa, in "Proceeding
of the 20th Stellar Conference, J. Du¹ek, M. Zejda (eds.), Brno, p97
- Pribulla, T., Chochol, D.: 1998, Period change in the contact
system AW UMa, Odessa Astronomical Publications 9, 43.
- Pribulla, T.: 1998, Efficiency of the mass transfer and outflow
in close binaries, Contrib. Astron. Obs. Skalnaté Pleso 28,
101.
ADS
- Pribulla, T., Chochol, D., Parimucha, Š.: 1999, Period and light
curve study of the eclipsing contact binary SW Lac, Contrib. Astron.
Obs. Skalnaté Pleso 29, 111.
ADS
- Pribulla, T., Chochol, D., Rovithis-Livaniou, H., Rovithis, P.: 1999,
The contact binary AW Ursae Majoris as a member of a multiple
system, Astron. Astrophys. 345, 137.
Springer Verlag
- Parimucha, Š., Pribulla, T., Vaňko, M.: 2000, New photoelectric
light curves of AB And, Inf. Bull. Variable Stars, 4834
IBVS
- Pribulla, T., Chochol, D., Tremko, D., Parimucha, Š., Vaňko, M.,
Kreiner, J.M.: 2000, Period study of the contact system VW Cep,
Contrib. Astron. Obs. Skalnaté Pleso 30, 117.
ADS
- Pribulla, T., Parimucha, Š., Vaňko, M.: 2000, New photoelectric
light curves of VW Cephei, Inf. Bull. Variable Stars, 4847.
IBVS
- Chochol, D., van Houten, C.J., Pribulla, T., Grygar, J.: 2001, Analysis of multicolour light curves of the eclipsing binaries AQ Tuc
and AY Vel, Contrib. Astron. Obs. Skalnaté Pleso 31, 5.
ADS
- van Houten, C.J., Chochol, D., Pribulla, T., Grygar, J.: 2001, Multicolour photometry of the eclipsing binaries AQ Tuc and AY Vel,
Contrib. Astron. Obs. Skalnaté Pleso 31, 61.
- Pribulla, T., Vaňko, M., Chochol, D., Parimucha, Š.: 2001, Photoelectric photometry of the eclipsing contact binaries: EF Dra,
GW Cep and CW Cas, Contrib. Astron. Obs. Skalnaté Pleso 31,
26.
ADS
- Pribulla, T., Vaňko, M., Parimucha, Š.: 2001, New photoelectric
photometry of the neglected contact binary EP And, Inf. Bull.
Variable Stars, 5184.
IBVS
- Vaňko, M., Pribulla, T., Chochol, D., Parimucha, Š., Kim, C.H., Lee,
J.W., Han, J.Y.: 2001, Photoelectric and CCD photometry of
eclipsing contact binaries: UV Lyn, FU Dra and AH Aur, Contrib.
Astron. Obs. Skalnaté Pleso 31, 129.
- Vaňko, M., Pribulla, T.: 2001, First ground-based photometry and
preliminary photometric elements of contact binary DN Cam, Inf.
Bull. Variable Stars, 5200.
IBVS
Detached binaries and multiple systems
Top of the page
- Chochol, D., Pribulla, T., Rovithis-Livaniou, H., Rovithis, P.,
Kranidiotis, A.: 1998, Photometric study of the eclipsing binary
EG Cep, Contrib. Astron. Obs. Skalnaté Pleso 28, 51.
ADS
- Chochol, D., Pribulla, T., Teodorani, M., Errico, L., Vittone, A.A.,
Milano, L., Barone, F.: 1998, The RS CVn binary XY UMa as a
member of a triple system, Astron. Astrophys. 340, 415.
Springer Verlag
- Rovithis-Livaniou, H., Rovithis, P., Kranidiotis, A.N., Chochol, D.,
Pribulla, T.: 1998, On the orbital period changes of EG Cep,
Inf. Bull. Variable Stars, 4563.
IBVS
- Horak, T.B., Grygar, J., van Houten, C.J., Chochol, D., Pribulla, T.:
1999, Photometric elements of the eclipsing binaries ZZ Cru, RU
Gru and DT Lup from multicolour light curves, Contrib. Astron. Obs.
Skalnaté Pleso 29, 127.
ADS
- Pribulla, T., Chochol, D., Parimucha, Š.: 1999, Photoelectric
minima of some eclipsing systems, Inf. Bull. Variable Stars, 4751
IBVS
- Pribulla, T., Chochol, D., Milano, L., Errico, L., Vittone, A.A.,
Barone, F., Parimucha, Š.: 2000, Active eclipsing binary RT
Andromedae revisited, Astron. Astrophys. 362, 169.
Springer Verlag
- Komzík, R., Ulla, A., Pribulla, T., Chochol, D., Grygar, J.: 2001,
Detection of the secondary minima in TX UMa, Inf. Bull.
Variable Stars, 5155.
IBVS
- Pribulla, T., Chochol, D., Heckert, P.A., Errico, L., Vittone, A.A.,
Parimucha, Š., Teodorani, M.: 2001, An active binary XY UMa
revisited, Astron. Astrophys. 371, 997.
EDP Sciences
- Pribulla, T., Vaňko, M., Parimucha, Š., Chochol, D.: 2001, New
photoelectric minima and updated ephemerides of selected Eclipsing
binaries, Inf. Bull. Variable Stars, 5056.
IBVS
Symbiotic stars and related objects
Top of the page
- Hric, L., Skopal, A., Urban, Z., Petrík, K., Komžík, R., Chochol, D., Pribulla,
T., Niarchos, P., Rovithis-Livaniou, H., Rovithis, P., Velič, Z., Okša, G.:
1996, Photometry of symbiotic stars - an international campaign VIIa,
Contrib. Astron. Obs. Skalnaté Pleso 26, 46
ADS
- Hric, L., Skopal, A., Urban, Z., Petrík, K., Komžík, R., Chochol, D., Pribulla,
T., Niarchos, P., Rovithis-Livaniou, H., Rovithis, P., Kaserkevitch, V.S.,
Shpychka, I.V., Velič, Z., Halevin, A.V., Andronov, I.L., Okša, G., Krtička, J.:
1996, Photometry of symbiotic stars - an international campaign VIIb,
Contrib. Astron. Obs. Skalnaté Pleso 26, 121
ADS
- Chochol, D., Tamura, S., Kanamitsu, O., Pribulla, T., Tajitsu, A.: 1996,
A close look at the outburst of the very slow symbiotic nova PU VUL - a
triple system, in "Cataclysmic Variables and related objects", A. Evans &
J.H. Wood (eds.), Kluwer, Dordrecht, p343
- Chochol, D., Tamura, S., Kanamitsu, O., Pribulla, T., Tajitsu, A.:
1997, Physical processes in the very slow symbiotic nova PU Vul
- possible triple system, in "Physical processes in symbiotic binaries
and related objects", J. Mikolajewska (ed.), Copernicus Foundation
for Polish Astronomy, Warsawa, p127
- Chochol, D., Pribulla, T., Tamura, S.: 1998, Pulsating AGB star
in the symbiotic nova PU Vulpeculae, Inf. Bull. Variable Stars, 4571
IBVS
- Chochol, D., Pribulla, T.: 2000, Pulsation of the AGB Variable
in the symbiotic Nova PU Vulpeculae, in: The impact of
Large-Scale Surveys on Pulsating Star Research, eds. L. Szabados,
D.W. Kurtz, Astronomical Society of the Pacific, San Francisco, p.
125.
- Parimucha, Š., Arkhipova, V.P., Chochol, D., Kroll, P., Pribulla, T.,
Shugarov, S.Yu., Ulyanikhina, O., Chinarova, L.L.: 2000, Long-term photometry of the symbiotic nova V1016 Cyg, Contrib.
Astron. Obs. Skalnaté Pleso 30, 99.
ADS
- Skopal, A., Chochol, D., Pribulla, T., Vaňko, M.: 2000, UBV
photometry of the symbiotic star Z And during its 2000 outburst,
Inf. Bull. Variable Stars., 5005.
IBVS
- Skopal, A., Pribulla, T., Wolf, M., Shugarov, S.Yu., Jones, A.: 2000,
Photometry of symbiotic stars IX. TX CVn, CH Cyg, AX Per and AR
Pav, Contrib. Astron. Obs. Skalnaté Pleso 30, 29.
ADS
Classical novae
Top of the page
- Chochol, D., Pribulla, T.: 1996, UBVR photometry of Nova
Cassiopeiae 1995, in "Physical Processes in Interacting Binaries",
D. Chochol et al. (eds.), Astronomical Institute of the SAS, Tatranska
Lomnica, p35
- Chochol, D., Grygar, J., Pribulla, T., Komžík, R., Hric, L., Elkin,
V.: 1997, The expansion of the envelope of Nova V1974 Cyg and
the distance problem, Astron. Astrophys. 318, 908.
Springer Verlag
- Chochol, D., Pribulla, T.: 1997, Photometric study of Nova Cas
1995, Contrib. Astron. Obs. Skalnaté Pleso 27, 53.
- Chochol, D., Pribulla, T.: 1998, Photometric variability of the
slow nova V723 Cas, Contrib. Astron. Obs. Skalnaté Pleso 28,
121.
ADS
- Chochol, D., Pribulla, T.: 1998, Shaping of the nova shells -
the case of nova V1974 Cygni, Odessa Astronomical Publications 9, 24.
- Chochol, D., Pribulla, T., Shemmer, O., Retter, A., Shugarov, S.Yu.,
Goranskij, V.P., Katysheva, M.A.: 2000, V723 Cassiopeiae, IAU
Circ., 7351
- Goranskij, V.P., Shugarov, S.Y., Katysheva, N.A., Shemmer, O., Retter, A.,
Chochol, D., Pribulla, T.: 2000, Orbital Period and Oscillations in
V723 Cassiopeiae, Inf. Bull. Variable Stars, 4852.
IBVS
Editation of the proceedings
Top of the page
- Chochol, D., Skopal, A., Pribulla, T.: 1996, Physical Processes in interacting
Binaries , Astronomical Institute of the Slovak Academy of Sciences and
Slovak Astronomical Society, Tatranská Lomnica
Files:
PS document
PDF document
My ADS query
Top of the page
Dissertation
Photometric and spectroscopic research of the contact binary system AW UMa
(in Slovak language)
Abstract
The main goal of this thesis was to determine basic characteristics of the
components of AW UMa contact binary and find the cause of the light curve
and orbital period changes. Another aim of the work was to prove or
disaprove possible existence of the third body and to found simple but
consistent model of the system.
The investigation presented in this work was based on a large photometric
and spectroscopic material obtained partly by the author and his supervisor.
The most important results of the work are:
- Finding that the outflow of matter from L$_2$ and resulting
angular momentum loss is the principal cause of the long term period
decrease.
- Discovery of the systemic velocity changes and finding of the
solution for the third body with the orbital period of 398 days, which
explains both systemic velocity changes and the variations found in
(O--C)$_2$ diagram.
- Transitions from the quiescent to active phase of the contact system
can be explained
by the tidal forces exerted by the common influence of the third body and
fourth body with the orbital period of 16.85 years (found from the
light-time
effect). This solution is supported by the pronounced variations of the
light
curve following the periastron passage of the fourth body.
Basic characteristics of the components of the quadrupole system AW UMa
were found. Masses of the components of the contact system set AW UMa on
the Zero Age Main Sequence.
Complete dissertation
Autoreferat
Submitted papers:
T. Pribulla, J.M. Kreiner, J. Tremko:
"Catalogue of the field contact binary stars" (sumbitted to
CAOSP)
Abstract:
The catalogue of 361 galactic contact binaries is presented. Enlisted
contact binaries are divided into five groups according to the type and
quality of the available observations and parameters. For all systems the
ephemeris for the primary minimum, minimum and maximum visual brightness
and
equatorial coordinates are given. If available, photometric elements,
$(m_1 + m_2) \sin^3 i$, spectral type, parallax and magnitude of the
O'Connell
effect are also given. Photometric data for several systems are augmented
by
new observations. The quality of the available data is assessed and
systems requiring modern light-curve solutions are selected.
Selected statistical properties of the collected data are discussed.
Postscript version of the paper
Last modified: November 18, 2002
Top of the page