Zobrazeno 1 - 10
of 11
pro vyhledávání: '"I. B. Biro"'
Autor:
I. Csányi, Krisztián Vida, János Bartus, Katalin Oláh, Zs. Kővári, Z. Csubry, Gáspár Á. Bakos, Saul Rappaport, D. W. Latham, Allyson Bieryla, Andrew Vanderburg, Joel D. Hartman, Waqas Bhatti, Daryll LaCourse, Mark Omohundro, Tamás Borkovits, I. B. Biro, Tom Jacobs
Publikováno v:
Astronomy & Astrophysics. 620:A189
Context. Stars can maintain their observable magnetic activity from the PMS to the tip of the red giant branch. However, the number of known active giants is much lower than active stars on the main sequence since on the giant branch the stars spend
Autor:
V. B. Kostov, S. A. Rappaport, T. Borkovits, B. P. Powell, R. Gagliano, M. Omohundro, I. B. Bíró, M. Moe, S. B. Howell, T. Mitnyan, C. A. Clark, M. H. Kristiansen, I. A. Terentev, H. M. Schwengeler, A. Pál, A. Vanderburg
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 1, p 25 (2024)
We have discovered a triply eclipsing triple-star system, TIC 290061484, with the shortest known outer period, P _out , of only 24.5 days. This “eclipses” the previous record set by λ Tauri at 33.02 days, which held for 68 yr. The inner binary,
Externí odkaz:
https://doaj.org/article/b0d2e21f7c1043f7b19db34a00a0869f
Autor:
Al Levine, I. B. Biro, T. Hajdu, Tamás Borkovits, Saul Rappaport, Peter Klagyivik, J. Sztakovics
We produce and analyze eclipse time variation (ETV) curves for some 2600 Kepler binaries. We find good to excellent evidence for a third body in 222 systems via either the light-travel-time (LTTE) or dynamical effect delays. Approximately half of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af821a1b114c3bc0aa1267e81bdc373d
http://arxiv.org/abs/1510.08272
http://arxiv.org/abs/1510.08272
Autor:
B. Csák, Róbert Szabó, D. W. Kurtz, John Southworth, J. Sztakovics, Aliz Derekas, Krešimir Pavlovski, József Kovács, Á. Dózsa, Tamás Borkovits, F. Maloney, I. B. Biro, Jim Fuller, Andrej Prsa, Gy. M. Szabó, Kelly Hambleton, V. Kolbas, Karen Kinemuchi, I. Jankovics
Publikováno v:
EPJ Web of Conferences, Vol 101, p 06021 (2015)
KIC 8560861 (HD 183648) is a marginally eccentric (e=0.05) eclipsing binary with an orbital period of P_orb=31.973d, exhibiting mmag amplitude pulsations on time scales of a few days. We present the results of the complex analysis of high and medium-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::309965d188048cadf2633eb6bd71f7a1
https://clok.uclan.ac.uk/14607/1/14607_epjconf_sphr2014_06021.pdf
https://clok.uclan.ac.uk/14607/1/14607_epjconf_sphr2014_06021.pdf
Autor:
J. Nuspl, T. Hegedüs, R. Csorvási, Sz. Csizmadia, Tamás Borkovits, I. B. Biro, M. M. Elkhateeb
Publikováno v:
Astronomy & Astrophysics. 441:1087-1097
Complex period variations of five W UMa type binaries (AB And, OO Aql, DK Cyg, V566 Oph, U Peg) were investigated by analyzing their O--C diagrams, and several common features were found. Four of the five systems show secular period variations at a c
Publikováno v:
Astronomy & Astrophysics. 392:895-907
Results of a new light-curve analysis and period variation study of the eclipsing binary IM Aur are presented. Four solutions are given according to the dierent spectral types of the primary, available in the literature. Multicolour photometry and th
Autor:
Tamás Borkovits, Daniel Huber, Amanda Király, I. B. Biro, Emese Forgács-Dajka, Róbert Szabó, Stephen T. Bryson, Aliz Derekas, Timothy R. Bedding, László L. Kiss
Publikováno v:
MON NOT R ASTRON SOC MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY.
HD 181068 is the brighter of the two known triply eclipsing hierarchical triple stars in the Kepler field. It has been continuously observed for more than 2 years with the Kepler space telescope. Of the nine quarters of the data, three have been obta
EM Cygni is a Z Cam-subtype eclipsing dwarf nova. Its orbital period variations were reported in the past but the results were in conflict to each other while other studies allowed the possibility of no period variation. In this study we report accur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa8a95be332579faa45a732bded2dd31
http://arxiv.org/abs/0709.2649
http://arxiv.org/abs/0709.2649
Autor:
Jozsef Vinko, Sz. Csizmadia, B. Csák, László L. Kiss, Gy. M. Szabó, Krisztián Sárneczky, K. Sziladi, G. Furesz, I. B. Biro
Publikováno v:
Scopus-Elsevier
CCD-photometry and low-resolution spectroscopy of the bright supernova SN 2000E in NGC 6951 are presented. Both the light curve extending up to 150 days past maximum and the spectra obtained at 1 month past maximum confirm that SN 2000E is of Type Ia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c2cf9b108eefa21dc9329225c1476f2
Autor:
E. Szegedi-Elek, Tamás Szalai, Károly Szatmáry, László L. Kiss, G. H. Marion, Tamás Kovács, A. Farkas, K. Takats, Krisztián Sárneczky, R. Szakats, T. Hegedüs, John C Wheeler, Jozsef Vinko, P. Klagyivik, A. Pál, K. Vida, N. Szalai, A. Szing, I. B. Biro, Tamás Borkovits
Publikováno v:
Astronomy & Astrophysics. 546:A12
The nearby, bright, almost completely unreddened Type Ia supernova 2011fe in M101 provides a unique opportunity to test both the precision and the accuracy of the extragalactic distances derived from SNe Ia light curve fitters. We apply the current,