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On the kinematic age of RZ Psc. / Potravnov, I.S.; Grinin, V.P.

в: Astronomy Letters, № 11, 2013, стр. 776-780.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Potravnov, IS & Grinin, VP 2013, 'On the kinematic age of RZ Psc', Astronomy Letters, № 11, стр. 776-780. https://doi.org/10.1134/S1063773713100058

APA

Potravnov, I. S., & Grinin, V. P. (2013). On the kinematic age of RZ Psc. Astronomy Letters, (11), 776-780. https://doi.org/10.1134/S1063773713100058

Vancouver

Potravnov IS, Grinin VP. On the kinematic age of RZ Psc. Astronomy Letters. 2013;(11):776-780. https://doi.org/10.1134/S1063773713100058

Author

Potravnov, I.S. ; Grinin, V.P. / On the kinematic age of RZ Psc. в: Astronomy Letters. 2013 ; № 11. стр. 776-780.

BibTeX

@article{14cc133c03144820929951e87c1cc851,
title = "On the kinematic age of RZ Psc",
abstract = "RZ Psc belongs to the family of young UX Ori stars whose photometric activity is due to strong extinction variations in the circumstellar disks surrounding them. However, in contrast to all the remaining stars of this type, no evidence of youth has been detected for RZ Psc until recently. A rough estimate of the star's kinematic age was made for the first time in our previous paper (Grinin et al. 2010). It shows that RZ Psc is intermediate in its evolutionary status between young stars in Orion and stars with debris disks. In this paper, we provide a refined estimate of the kinematic age for the star confirming this conclusion. According to this estimate, the age of RZ Psc is approximately 25 ± 5 Myr at M * = 1M ⊙. {\textcopyright} 2013 Pleiades Publishing, Inc.",
author = "I.S. Potravnov and V.P. Grinin",
year = "2013",
doi = "10.1134/S1063773713100058",
language = "English",
pages = "776--780",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "11",

}

RIS

TY - JOUR

T1 - On the kinematic age of RZ Psc

AU - Potravnov, I.S.

AU - Grinin, V.P.

PY - 2013

Y1 - 2013

N2 - RZ Psc belongs to the family of young UX Ori stars whose photometric activity is due to strong extinction variations in the circumstellar disks surrounding them. However, in contrast to all the remaining stars of this type, no evidence of youth has been detected for RZ Psc until recently. A rough estimate of the star's kinematic age was made for the first time in our previous paper (Grinin et al. 2010). It shows that RZ Psc is intermediate in its evolutionary status between young stars in Orion and stars with debris disks. In this paper, we provide a refined estimate of the kinematic age for the star confirming this conclusion. According to this estimate, the age of RZ Psc is approximately 25 ± 5 Myr at M * = 1M ⊙. © 2013 Pleiades Publishing, Inc.

AB - RZ Psc belongs to the family of young UX Ori stars whose photometric activity is due to strong extinction variations in the circumstellar disks surrounding them. However, in contrast to all the remaining stars of this type, no evidence of youth has been detected for RZ Psc until recently. A rough estimate of the star's kinematic age was made for the first time in our previous paper (Grinin et al. 2010). It shows that RZ Psc is intermediate in its evolutionary status between young stars in Orion and stars with debris disks. In this paper, we provide a refined estimate of the kinematic age for the star confirming this conclusion. According to this estimate, the age of RZ Psc is approximately 25 ± 5 Myr at M * = 1M ⊙. © 2013 Pleiades Publishing, Inc.

U2 - 10.1134/S1063773713100058

DO - 10.1134/S1063773713100058

M3 - Article

SP - 776

EP - 780

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 11

ER -

ID: 7520086