Astronomy with the BIMA Array

BIMA 阵列的天文学

• 批准号: 9613716
• 负责人: Stuart Vogel
• 金额: $ 47.11万
• 依托单位: University of Maryland, College Park
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 1997
• 资助国家: 美国
• 起止时间: 1997-01-01 至 2000-12-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9613716&HistoricalAwards=false
• 关键词: Astronomy; BIMA; Array

AST-96-13998. University of California at Berkeley. PI: - Blitz AST-96-13999. University of Illinois. PI: - E. Snyder AST-96-13716. University of Maryland. PI: - S. Vogel Astronomy with the BIMA Array The Berkeley-Illinois-Maryland Array (BIMA) is a millimeter-wave interferometer presently made up of 9 six-meter diameter antennas; at least two other antennas will be added to the array during the next 5 years. located at Berkeley's Hat Creek Radio Observatory, BIMA was jointly capitalized and is jointly operated by the University of California at Berkeley, the University of Illinois and the University of Maryland through a combination of NSF and State funding. These awards are for identical proposals submitted simultaneously by each institution, and support astronomical research, technological development and student training carried out at the BIMA array. Astronomical research at BIMA includes high resolution studies of solar system objects, stellar envelopes, star-forming regions in the Galaxy, and molecular clouds in external galaxies. Notable accomplishments during the past three years at BIMA include expansion from 6 to 9 elements, and the extension of the array baselines to provide angular resolutions better than 0.5 arcsecond. These technical advancements permitted BIMA scientists to obtain the first resolved image of a young circumstellar disk, and to discover a molecular bar at the core of the Seyfert galaxy NGC 1068, and to confirm the discovery of interstellar acetic acid. Scientific plans under the new award will focus heavily on exploiting the recently-achieved higher speed and resolution of the array. In the technical domain, BIMA staff will concentrate attempting to use total power fluctuations to remove the phase fluctuations caused by the atmosphere when operating over long baselines.

ast - 96 - 13998。加州大学伯克利分校。PI: -闪电战AST-96-13999伊利诺伊大学。PI: - E. Snyder AST-96-13716。马里兰大学。伯克利-伊利诺伊-马里兰阵列（BIMA）是一个毫米波干涉仪，目前由9个直径6米的天线组成；在接下来的5年里，至少还有两个天线将被添加到阵列中。BIMA位于伯克利的Hat Creek射电天文台，由加州大学伯克利分校、伊利诺伊大学和马里兰大学共同出资运营，由美国国家科学基金会和国家资助。这些奖项是针对每个机构同时提交的相同提案，并支持在BIMA阵列进行的天文研究、技术开发和学生培训。BIMA的天文研究包括对太阳系天体、恒星包层、银河系恒星形成区域和外部星系分子云的高分辨率研究。在过去的三年中，BIMA取得了显著的成就，包括从6个元素扩展到9个元素，以及扩展阵列基线以提供优于0.5角秒的角分辨率。这些技术进步使BIMA的科学家们获得了第一张年轻星周盘的分辨率图像，并在Seyfert星系ngc1068的核心发现了一个分子棒，并证实了星际乙酸的发现。新奖项下的科学计划将着重于开发最近实现的更高速度和分辨率的阵列。在技术领域，BIMA工作人员将集中精力，试图利用总功率波动来消除在长基线上运行时由大气引起的相位波动。