High Resolution Optical Spectra of HBC 722 after Outburst

Дата и время публикации : 2011-04-04T12:20:02Z

Авторы публикации и институты :
Jeong-Eun Lee
Wonseok Kang
Sang-Gak Lee
Hyun-Il Sung
Byeong-Cheol Lee
Hwankyung Sung
Joel D. Green
Young-Beom Jeon

Ссылка на журнал-издание: Ссылка на журнал-издание не найдена
Коментарии к cтатье: accepted for publication in JKAS
Первичная категория: astro-ph.SR

Все категории : astro-ph.SR

Краткий обзор статьи: We report the results of our high resolution optical spectroscopic monitoring campaign ($lambda$ = 3800 — 8800 A, R = 30000 — 45000) of the new FU Orionis-type object HBC 722. We observed HBC 722 with the BOES 1.8-m telescope between 2010 November 26 and 2010 December 29 and FU Orionis itself on 2011 January 26. We detect a number of previously unreported high-resolution K I and Ca II lines beyond 7500 A. We resolve the H$alpha$ and Ca II line profiles into three velocity components, which we attribute to both disk and outflow. The increased accretion during outburst can heat the disk to produce the relatively narrow absorption feature and launch outflows appearing as high velocity blue and redshifted broad features.

Category: Physics