HIGH-SPEEDBULLETEJECTIONSDURINGTHEAGB-TO-PLANETARY.pdfVIP

HIGH-SPEEDBULLETEJECTIONSDURINGTHEAGB-TO-PLANETARY.pdf

  1. 1、本文档共13页,可阅读全部内容。
  2. 2、原创力文档(book118)网站文档一经付费(服务费),不意味着购买了该文档的版权,仅供个人/单位学习、研究之用,不得用于商业用途,未经授权,严禁复制、发行、汇编、翻译或者网络传播等,侵权必究。
  3. 3、本站所有内容均由合作方或网友上传,本站不对文档的完整性、权威性及其观点立场正确性做任何保证或承诺!文档内容仅供研究参考,付费前请自行鉴别。如您付费,意味着您自己接受本站规则且自行承担风险,本站不退款、不进行额外附加服务;查看《如何避免下载的几个坑》。如果您已付费下载过本站文档,您可以点击 这里二次下载
  4. 4、如文档侵犯商业秘密、侵犯著作权、侵犯人身权等,请点击“版权申诉”(推荐),也可以打举报电话:400-050-0827(电话支持时间:9:00-18:30)。
  5. 5、该文档为VIP文档,如果想要下载,成为VIP会员后,下载免费。
  6. 6、成为VIP后,下载本文档将扣除1次下载权益。下载后,不支持退款、换文档。如有疑问请联系我们
  7. 7、成为VIP后,您将拥有八大权益,权益包括:VIP文档下载权益、阅读免打扰、文档格式转换、高级专利检索、专属身份标志、高级客服、多端互通、版权登记。
  8. 8、VIP文档为合作方或网友上传,每下载1次, 网站将根据用户上传文档的质量评分、类型等,对文档贡献者给予高额补贴、流量扶持。如果你也想贡献VIP文档。上传文档
查看更多
HIGH-SPEEDBULLETEJECTIONSDURINGTHEAGB-TO-PLANETARY

The Astrophysical Journal, 827:92 (13pp), 2016 August 20 ? 2016. The American Astronomical Society. All rights reserved. doi:10.3847/0004-637X/827/2/92 HIGH-SPEED BULLET EJECTIONS DURING THE AGB-TO-PLANETARY NEBULA TRANSITION: HST OBSERVATIONS OF THE CARBON STAR, V HYDRAE 1 1,2 3 R. Sahai , S. Scibelli , and M. R. Morris 1 Jet Propulsion Laboratory, MS 183-900, California Institute of Technology, Pasadena, CA 91109, USA; raghvendra.sahai@jpl.nasa.gov 2 Stony Brook University, Stony Brook, NY 11794-3800, USA 3 Department of Physics and Astronomy, UCLA, Los Angeles, CA 90095-1547, USA Received 2016 March 22; revised 2016 May 18; accepted 2016 May 19; published 2016 August 11 ABSTRACT The well-studied carbon star, V Hya, showing evidence for high-speed, collimated out?ows and dense equatorial structures, is a key object in the study of the poorly understood transition of AGB stars into aspherical planetary nebulae. Using the Space Telescope Imaging Spectrograph instrument on board the Hubble Space Telescope, we have obtained high spatial-resolution long-slit optical spectra of V Hya that show high-velocity emission in [S II] and [Fe II] lines. Our data set, spanning three epochs spaced apart by a year during each of two periods (in 2002–2004 and 2011–2013), shows that V Hya ejects high-speed (~200–250 km s-1) bullets once every ~8.5 years. The ejection axis ?ip–?ops around a roughly eastern direction, both in and perpendicular to the skyplane, and the radial velocities of the ejecta also vary in concert between low and high values. We propose a model in which the bullet ejection is associated with the periastron passage of a binary companion in an eccentric orbit around V Hya with an orbital period of ~8.5 years. The ?ip–?op phenomenon is likely the result of collimated ejection from an accretion disk (produced by gravitational capture of material from the primary) that is warped and precessing, and/or that has a magnetic ?eld that is misaligned with that of the compan

文档评论(0)

***** + 关注
实名认证
文档贡献者

该用户很懒,什么也没介绍

版权声明书
用户编号:8010045112000002

1亿VIP精品文档

相关文档