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Surprising variations in the rotation of the chemically peculiar stars CU Virginis and V901 Orionis
Názov Surprising variations in the rotation of the chemically peculiar stars CU Virginis and V901 Orionis Spoluautori Mikulášek Zdeněk Krtička Jiří Henry Gregg W. Janík Jan Zverko Juraj SAVASTRO - Astronomický ústav SAV Žižňovský Jozef SAVASTRO - Astronomický ústav SAV Zejda Miloš Liška Jiří Zvěřina Pavel Kudryavtsev Dmitrij O. Romanyuk Iosif I. Sokolov Nikolay A. Lüftinger Theresa Trigilio Corrado Neiner Coralie de Villiers S.N. Zdroj.dok. Astronomy and Astrophysics. Vol. 534 (2011), article no. L5, p. 1-5 Jazyk dok. eng - angličtina Krajina FR - Francúzsko Druh dok. rozpis článkov z periodík (rbx) Ohlasy PAUNZEN, E. - WRAIGHT, K. T. - FOSSATI, L. - NETOPIL, M. - WHITE, G. J. - BEWSHER, D. A photometric study of chemically peculiar stars with the STEREO satellites II. Non-magnetic chemically peculiar stars. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, vol. 429, no. 1, p. 119-125. PYPER, D.M. - STEVENS, I.R. - ADELMAN, S.J. An update on the rotational period of the magnetic chemically peculiar star CU Virginis. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, vol. 431, no. 3, p. 2106-2110. PETIT, V. - OWOCKI, S. P. - WADE, G. A. - COHEN, D. H. - SUNDQVIST, J. O. - GAGNE, M. - MAIZ APELLANIZ, J. - OKSALA, M. E. - BOHLENDER, D. A. - RIVINIUS, T. - HENRICHS, H. F. - ALECIAN, E. - TOWNSEND, R. H. D. - UD-DOULA, A. A magnetic confinement versus rotation classification of massive-star magnetospheres. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, vol. 429, no. 1, p. 398-422. SHULTZ, M. - WADE, G. A. Confirming the oblique rotator model for the extremely slowly rotating O8f?p star HD 108. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. ISSN 0035-8711, 2017, vol. 468, no. 4, p. 3985-3992. BRAITHWAITE, J. - SPRUIT, H. C. Magnetic fields in non-convective regions of stars. In ROYAL SOCIETY OPEN SCIENCE. ISSN 2054-5703, 2017, vol. 4, no. 2, article no. 160271, p. 1-45. KOCHUKHOV, O. - SILVESTER, J. - BAILEY, J. D. - LANDSTREET, J. D. - WADE, G. A. Magnetic field topology and chemical abundance distributions of the young, rapidly rotating, chemically peculiar star HR5624. In ASTRONOMY AND ASTROPHYSICS. ISSN 1432-0746, 2017, vol. 605, article no. A13, p. 1-17. SHULTZ, M. - RIVINIUS, T. - DAS, B. - WADE, G. A. - CHANDRA, P. The accelerating rotation of the magnetic He-weak star HD 142990. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. ISSN 0035-8711, 2019, vol. 486, no. 4, p. 5558-5566. DAS, B. - CHANDRA, P. - SHULTZ, M. E. - WADE, G. A. Detection of coherent emission from the Bp star HD 142990 at uGMRT frequencies. In ASTROPHYSICAL JOURNAL. ISSN 0004-637X, 2019, vol. 877, no. 2, article no. 123, p. 1-12. DAS, Barnali - CHANDRA, Poonam - WADE, Gregg A. Unravelling the complex magnetosphere of the B star HD 133880 via wideband observation of coherent radio emission. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. ISSN 0035-8711, 2020, vol. 499, no. 1, p. 702-709. BERNHARD, Klaus - HUEMMERICH, Stefan - PAUNZEN, Ernst. New and improved rotational periods of magnetic CP stars from ASAS-3, KELT, and MASCARA data. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. ISSN 0035-8711, 2020, vol. 493, no. 3, p. 3293-3330. PYPER, Diane M. - ADELMAN, Saul J. Newly discovered period changes in two mCP stars and updates for previously published stars. In PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC. ISSN 0004-6280, 2020, vol. 132, no. 1008, article no. 024201, p. 1-18. KESZTHELYI, Z. - MEYNET, G. - SHULTZ, M. E. - DAVID-URAZ, A. - UD-DOULA, A. - TOWNSEND, R. H. D. - WADE, G. A. - GEORGY, C. - PETIT, V - OWOCKI, S. P. The effects of surface fossil magnetic fields on massive star evolution II. Implementation of magnetic braking in MESA and implications for the evolution of surface rotation in OB stars. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. ISSN 0035-8711, 2020, vol. 493, no. 1, p. 518-535. DAS, Barnali - CHANDRA, Poonam. Ultra-wideband, multiepoch radio study of the first discovered "Main-sequence Radio Pulse Emitter" CU Vir. In ASTROPHYSICAL JOURNAL. ISSN 0004-637X, 2021, vol. 921, no. 1, article no. 9, p. 1-20. Dostupné na: https://doi.org/10.3847/1538-4357/ac1075. PYPER, Diane M. - ADELMAN, Saul J. Light curve changes and possible precession in mCP stars. In PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC. ISSN 0004-6280, 2021, vol. 133, no. 1026, article no. 084203, p. 1-18. Dostupné na: https://doi.org/10.1088/1538-3873/ac1ac0. SHULTZ, M. E. - ALECIAN, E. - PETIT, V - BAGNULO, S. - BOHM, T. - FOLSOM, C. P. - WADE, G. A. NGC6611601: a hot pre-main-sequence spectroscopic binary containing a centrifugal magnetosphere host star. In MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. ISSN 0035-8711, 2021, vol. 504, no. 3, pp. 3203-3220. Dostupné na: https://doi.org/10.1093/mnras/stab822. HUBRIG, Swetlana - SCHOELLER, Markus. MAGNETIC FIELDS IN O, B, AND A STARS. Bristol: IOP Publishing, 2021. 212 p. ISBN 978-0-7503-2390-1. Dostupné na: https://doi.org/10.1088/2514-3433/abefcc. SONG, H. F. - MEYNET, G. - MAEDER, A. - MOWLAVI, N. - STROUD, S. R. - KESZTHELYI, Z. - EKSTROM, S. - EGGENBERGER, P. - GEORGY, C. - WADE, G. A. - QIN, Y. News from Gaia on sigma Ori E: A case study for the wind magnetic braking process. In ASTRONOMY AND ASTROPHYSICS, 2022, vol. 657, article no. A60, p. 1-13. ISSN 0004-6361. Dostupné na: https://doi.org/10.1051/0004-6361/202141512. KESZTHELYI, Zsolt. Magnetism in high-mass stars. In GALAXIES, 2023, vol. 11, no. 2, article no. 40, p. 1-26. ISSN 2075-4434. Dostupné na: https://doi.org/10.3390/galaxies11020040. Kategória ADCA - Vedecké práce v zahraničných karentovaných časopisoch impaktovaných Kategória (od 2022) V3 - Vedecký výstup publikačnej činnosti z časopisu Typ výstupu článok Rok vykazovania 2011 Registrované v WOS Registrované v SCOPUS Registrované v CCC DOI 10.1051/0004-6361/201117784 článok
rok CC IF IF Q (best) JCR Av Jour IF Perc SJR SJR Q (best) CiteScore A rok vydania rok metriky IF IF Q (best) SJR SJR Q (best) 2011 2010 4.425 Q1 2.849 Q1
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