Conference support: A Population Explosion: The Nature and Evolution of X-ray Binaries in Diverse Environments; Oct.28-Nov.2 2007; St.Petersburg, FL

会议支持：人口爆炸：不同环境中 X 射线双星的性质和演化；

• 批准号: 0715299
• 负责人: Reba Bandyopadhyay
• 金额: --
• 依托单位: University of Florida
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2007
• 资助国家: 美国
• 起止时间: 2007-06-15 至 2008-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0715299&HistoricalAwards=false
• 关键词: Conference; support; Population; Explosion; Nature

This award will provide financial support for the international conference A Population Explosion: The Nature and Evolution of X-ray Binaries in Diverse Environments to be held in St. Petersburg Beach, Florida, 28 October to 2 November 2007.This conference is focused on the dramatic increase in the number and variety of known x-ray binaries and the need to take a broader look at the binary population, including the feedback and interaction with the environment, both within our Galaxy and in external systems. In particular, the organizers will highlight information obtained from observations at "non-traditional" wavelengths, especially the infrared, and to explore how the current and future large scale surveys at various wavelengths will contribute to the understanding of the X-ray binary population and their environment.The scientific program is organized along five topics (one per day):. X-ray binary jets and outflows in high and low X-ray luminosity systems . Galactic Center accreting binary population . Obscured populations, INTEGRAL sources, and supergiant fast X-ray transients . Extragalactic X-ray binary populations and ultraluminous X-ray sources . X-ray binary population synthesis and stellar evolutionThe meeting is designed with an emphasis on discussion. Attendance will be limited to 150 participants. To facilitate this discussion, an extra 30 minutes will be scheduled per session to allow discussions to continue past the nominal allocated time after invited and contributed talks. Poster presenters will also be encouraged to present a single slide summary of their poster in the middle of each appropriate topical session. The proceedings will be made available to the community and general public through electronic means, namely the The Smithsonian/NASA Astrophysics Data System, the Cornell University Library astrophysics preprint server (astro-ph), and online journals. Full texts of the proceedings will be available through Astrophysics Data System. Edited CDs of the proceedings will also be distributed to all participants.

该奖项将为国际会议提供财政支持人口爆炸：2007年10月28日至11月2日在佛罗里达州的彼得堡海滩举行的X射线双星在不同环境中的性质和演化会议。包括反馈和与环境的互动，无论是在我们的银河系内部还是外部系统。特别是，组织者将重点介绍从“非传统”波长，特别是红外线观测中获得的信息，并探索当前和未来各种波长的大规模调查将如何有助于了解X射线双星群及其环境。科学计划按沿着五个主题组织（每天一个）：。在高和低X射线光度系统中X射线双星喷流和外流。银河系中心吸积双星。模糊的星群、积分源和超巨星快速X射线瞬变。河外X射线双星群和超亮X射线源。X射线双星布居合成与恒星演化会议以讨论为主。出席人数将限于150人。为了方便讨论，每次会议将安排额外的30分钟，以便在邀请和贡献的演讲之后，讨论能够继续超过名义分配的时间。还鼓励海报展示者在每个适当的专题会议中间展示一张海报的幻灯片摘要。会议记录将通过电子方式向社区和公众提供，即史密森尼/美国宇航局天体物理学数据系统，康奈尔大学图书馆天体物理学预印本服务器（astro-ph）和在线期刊。会议记录的全文将通过天体物理数据系统提供。还将向所有与会者分发经过编辑的会议记录光盘。