Standard

HD 158450: A Magnetic Chemically Peculiar Star in a Young Stellar Group. / Drake, N.A.; Jilinski, E.G.; Ortega, V.G.; de, La Reza R.; Bazzanella, B.

Odessa Astronomical Publications. 2008. стр. 35.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике › научная

Harvard

Drake, NA, Jilinski, EG, Ortega, VG, de, LRR & Bazzanella, B 2008, HD 158450: A Magnetic Chemically Peculiar Star in a Young Stellar Group. в Odessa Astronomical Publications. стр. 35. <http://adsabs.harvard.edu/abs/2008OAP....21...35D>

APA

Drake, N. A., Jilinski, E. G., Ortega, V. G., de, L. R. R., & Bazzanella, B. (2008). HD 158450: A Magnetic Chemically Peculiar Star in a Young Stellar Group. в Odessa Astronomical Publications (стр. 35) http://adsabs.harvard.edu/abs/2008OAP....21...35D

Vancouver

Drake NA, Jilinski EG, Ortega VG, de LRR, Bazzanella B. HD 158450: A Magnetic Chemically Peculiar Star in a Young Stellar Group. в Odessa Astronomical Publications. 2008. стр. 35

Author

Drake, N.A. ; Jilinski, E.G. ; Ortega, V.G. ; de, La Reza R. ; Bazzanella, B. / HD 158450: A Magnetic Chemically Peculiar Star in a Young Stellar Group. Odessa Astronomical Publications. 2008. стр. 35

BibTeX

@inbook{ecc8059d84264fe59d100ccad813c4de,
title = "HD 158450: A Magnetic Chemically Peculiar Star in a Young Stellar Group",
abstract = "We report on the discovery of the Zeeman resolved spectral lines, corresponding to the very large magnetic field modulus [H] = 11.1 kG, in the spectrum of the chemically peculiar star HD 158450 belonging to the recently discovered Mamajek 2 stellar group. We determined fundamental parameters and projected rotation velocity of the star. Dynamical 3D mean orbit calculations showed that Mamajek 2 stellar group has an age of 135+-5 Myr. Based on this age, we estimate that HD 158450 has completed about 12% of its main-sequence life. The importance of the detailed study of HD 158450, a member of a stellar group with a well determined age, for understanding the origin and evolution of stellar magnetic fields is discussed.",
author = "N.A. Drake and E.G. Jilinski and V.G. Ortega and de, {La Reza R.} and B. Bazzanella",
year = "2008",
language = "не определен",
pages = "35",
booktitle = "Odessa Astronomical Publications",

}

RIS

TY - CHAP

T1 - HD 158450: A Magnetic Chemically Peculiar Star in a Young Stellar Group

AU - Drake, N.A.

AU - Jilinski, E.G.

AU - Ortega, V.G.

AU - de, La Reza R.

AU - Bazzanella, B.

PY - 2008

Y1 - 2008

N2 - We report on the discovery of the Zeeman resolved spectral lines, corresponding to the very large magnetic field modulus [H] = 11.1 kG, in the spectrum of the chemically peculiar star HD 158450 belonging to the recently discovered Mamajek 2 stellar group. We determined fundamental parameters and projected rotation velocity of the star. Dynamical 3D mean orbit calculations showed that Mamajek 2 stellar group has an age of 135+-5 Myr. Based on this age, we estimate that HD 158450 has completed about 12% of its main-sequence life. The importance of the detailed study of HD 158450, a member of a stellar group with a well determined age, for understanding the origin and evolution of stellar magnetic fields is discussed.

AB - We report on the discovery of the Zeeman resolved spectral lines, corresponding to the very large magnetic field modulus [H] = 11.1 kG, in the spectrum of the chemically peculiar star HD 158450 belonging to the recently discovered Mamajek 2 stellar group. We determined fundamental parameters and projected rotation velocity of the star. Dynamical 3D mean orbit calculations showed that Mamajek 2 stellar group has an age of 135+-5 Myr. Based on this age, we estimate that HD 158450 has completed about 12% of its main-sequence life. The importance of the detailed study of HD 158450, a member of a stellar group with a well determined age, for understanding the origin and evolution of stellar magnetic fields is discussed.

M3 - статья в сборнике

SP - 35

BT - Odessa Astronomical Publications

ER -

ID: 4503942