Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Viktor Khalack"'
Autor:
Swetlana Hubrig, Silva P. Järvinen, H. Adigozalzade, Ilya Ilyin, Viktor Khalack, Gautier Mathys
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 499:2734-2743
High resolution spectropolarimetric observations of the strongly magnetic, super-slowly rotating rapidly oscillating Ap star HD166473 are used to investigate the implications of the presence of a variable strong magnetic field on the vertical and sur
Autor:
A. David-Uraz, Ernst Paunzen, Viktor Khalack, Oleh Kobzar, Coralie Neiner, Oleg Kochukhov, J. Labadie-Bartz
Mercury-manganese (HgMn) stars are late-B upper main sequence chemically peculiar stars distinguished by large overabundances of heavy elements, slow rotation, and frequent membership in close binary systems. These stars lack strong magnetic fields t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02c4a934968c5b41171a1578b42e6925
http://arxiv.org/abs/2107.09096
http://arxiv.org/abs/2107.09096
Autor:
Aliz Derekas, N. Hatamkhani, D. W. Kurtz, T. Richey-Yowell, J. Pascual-Granado, P. Lampens, K. R. Pollard, Roland Vanderspek, A. García Hernández, Joyce A. Guzik, Ádám Sódor, Fangfei Shi, Catherine Lovekin, Zs. Bognár, Simon J. Murphy, Oleh Kobzar, Victoria Antoci, Viktor Khalack, Barry Smalley, A. Samadi-Ghadim, Dominic M. Bowman, A. David-Uraz, Derek Buzasi, E. Brunsden, M. Lares-Martiz, Oleg Kochukhov, Ivanka Stateva, T. Z. Yang, E. Niemczura, Dogus Ozuyar, Rasmus Handberg, P. Mikołajczyk, A. Ramón-Ballesta, T. S. Lambert, L. Fox-Machado, J. Sikora, P. Quitral-Manosalva, David Mkrtichian, Richard Monier, M. S. Cunha, Róbert Szabó, Daniel R. Hey, Daniel Luke Holdsworth, Ernst Paunzen
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digital.CSIC. Repositorio Institucional del CSIC
Holdsworth, D L, Cunha, M S, Kurtz, D W, Antoci, V, Hey, D R, Bowman, D M, Kobzar, O, Buzasi, D L, Kochukhov, O, Niemczura, E, Ozuyar, D, Shi, F, Szabó, R, Samadi-Ghadim, A, Bognár, Z, Fox-Machado, L, Khalack, V, Lares-Martiz, M, Lovekin, C C, Mikołajczyk, P, Mkrtichian, D, Pascual-Granado, J, Paunzen, E, Richey-Yowell, T, Sódor, Á, Sikora, J, Yang, T Z, Brunsden, E, David-Uraz, A, Derekas, A, Hernández, A G, Guzik, J A, Hatamkhani, N, Handberg, R, Lambert, T S, Lampens, P, Murphy, S J, Monier, R, Pollard, K R, Quitral-Manosalva, P, Ramón-Ballesta, A, Smalley, B, Stateva, I & Vanderspek, R 2021, ' TESS Cycle 1 observations of roAp stars with 2-min cadence data ', Monthly Notices of the Royal Astronomical Society, vol. 506, pp. 1073–1110 . https://doi.org/10.1093/mnras/stab1578
instname
Digital.CSIC. Repositorio Institucional del CSIC
Holdsworth, D L, Cunha, M S, Kurtz, D W, Antoci, V, Hey, D R, Bowman, D M, Kobzar, O, Buzasi, D L, Kochukhov, O, Niemczura, E, Ozuyar, D, Shi, F, Szabó, R, Samadi-Ghadim, A, Bognár, Z, Fox-Machado, L, Khalack, V, Lares-Martiz, M, Lovekin, C C, Mikołajczyk, P, Mkrtichian, D, Pascual-Granado, J, Paunzen, E, Richey-Yowell, T, Sódor, Á, Sikora, J, Yang, T Z, Brunsden, E, David-Uraz, A, Derekas, A, Hernández, A G, Guzik, J A, Hatamkhani, N, Handberg, R, Lambert, T S, Lampens, P, Murphy, S J, Monier, R, Pollard, K R, Quitral-Manosalva, P, Ramón-Ballesta, A, Smalley, B, Stateva, I & Vanderspek, R 2021, ' TESS Cycle 1 observations of roAp stars with 2-min cadence data ', Monthly Notices of the Royal Astronomical Society, vol. 506, pp. 1073–1110 . https://doi.org/10.1093/mnras/stab1578
We thank the anonymous referee for a careful reading of the manuscript. DLH acknowledges financial support from the Science and Technology Facilities Council (STFC) via grant ST/M000877/1. MSC acknowledges the support by FCT/MCTES through the researc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::14c04df5a1f169bc9b2c3e777df87226
http://hdl.handle.net/10481/71174
http://hdl.handle.net/10481/71174
Eclipsing binary stars are rare and extremely valuable astrophysical laboratories that make possible precise determination of fundamental stellar parameters. Investigation of early-type chemically peculiar stars in eclipsing binaries provides importa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4f47ef60d3c8e534f229af65a74cc03
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-458511
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-458511
How magnetic fields contribute to the differentiation of the rotation rates of the Ap stars and affect the occurrence of non-radial pulsation in some of them are important open questions. Valuable insight can be gained into these questions by studyin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70686cad30d22491f1a115a2112b1561
Autor:
Oleg Kochukhov, Daniel Luke Holdsworth, Patrick Lenz, Catherine Lovekin, Alexandre David-Uraz, Gregg A. Wade, Dominic M. Bowman, Oleh Kobzar, Viktor Khalack, James Sikora, Ernst Paunzen
Publikováno v:
Monthly Notices of the Royal Astronomical Society
The new photometric data on pulsating Ap star HD~27463 obtained recently with the Transiting Exoplanet Survey Satellite (\textit{TESS}) are analysed to search for variability. Our analysis shows that HD~27463 exhibits two types of photometric variabi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0526b6b2c04e7a11027486a97ffa46eb
https://lirias.kuleuven.be/handle/123456789/645535
https://lirias.kuleuven.be/handle/123456789/645535
Autor:
Adela Kawka, Lilia Ferrario, Stephane Vennes, Erek H. Alper, Péter Németh, John R. Thorstensen, Viktor Khalack
Publikováno v:
Science. 357:680-683
Subluminous Type Ia supernovae, such as the Type Iax class prototype SN 2002cx, are described by a variety of models such as the failed detonation and partial deflagration of an accreting carbon-oxygen white dwarf star, or the explosion of an accreti
Autor:
Ernst Paunzen, James Sikora, Oleh Kobzar, Coralie Neiner, Alexandre David-Uraz, Gregg A. Wade, S. Chowdhury, Oleg Kochukhov, Viktor Khalack, Dominic M. Bowman
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 487 (4), pp.4695-4710. ⟨10.1093/mnras/stz1581⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 487 (4), pp.4695-4710. ⟨10.1093/mnras/stz1581⟩
Recently, high-precision optical 2~min cadence light curves obtained with \emph{TESS} for targets located in the mission's defined first four sectors have been released. The majority of these high-cadence and high-precision measurements currently spa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c676349e41175cd48ef2a63484cc6846
https://lirias.kuleuven.be/handle/123456789/641285
https://lirias.kuleuven.be/handle/123456789/641285
Autor:
Dominic M. Bowman, Alexandre David-Uraz, Gregg A. Wade, Asif ud-Doula, Matt Shultz, Viktor Khalack, Stan Owocki, Matteo Cantiello, C. Neiner, M. Pergeorelis, C. Erba, R. MacInnis, Catherine Lovekin, Z. Keszthelyi, Oleh Kobzar, J. Labadie-Bartz, Herbert Pablo, S. Chowdhury, Gerald Handler, James Sikora, Véronique Petit, David H. Cohen, Oleg Kochukhov
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 487 (1), pp.304-317. ⟨10.1093/mnras/stz1181⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 487 (1), pp.304-317. ⟨10.1093/mnras/stz1181⟩
In this paper we introduce the MOBSTER collaboration and lay out its scientific goals. We present first results based on the analysis of nineteen previously known magnetic O, B and A stars observed in 2-minute cadence in sectors 1 and 2 of the Transi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c1e2ade6925ae1e1701af9aa52acd3c
https://lirias.kuleuven.be/handle/123456789/639785
https://lirias.kuleuven.be/handle/123456789/639785
Autor:
Richard Monier, Viktor Khalack
Publikováno v:
Research Notes of the AAS. 5:104
Abundances for 20 chemical elements are derived for Maia, the fourth brightest member of the Pleiades, using updated atomic data. Maia does not seem to be a typical helium-weak star nor a classical HgMn star. Instead Maia might be related to the phos