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Peculiar variations of white dwarf pulsation frequencies and maestro.

机译:白矮星脉动频率和大师的奇特变化。

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摘要

In Part I we report on variations of the normal mode frequencies of the pulsating DB white dwarfs EC 20058-5234 and KIC 8626021 and the pulsating DA white dwarf GD 66. The observations of EC 20058-5234 and KIC 8626021 were motivated by the possibility of measuring the plasmon neutrino production rate of a white dwarf, while the observations of GD 66 were part of a white dwarf pulsation timing based planet search. We announce the discovery of periodic and quasi-periodic variations of multiple normal mode frequencies that cannot be due to the presence of planetary companions. We note the possible signature of a planetary companion to EC 20058-5234 and show that GD 66 cannot have a planet in a several AU orbit down to half a Jupiter mass. We also announce the discovery of secular variations of the normal mode frequencies of all three stars that are inconsistent with cooling alone. Importantly, the rates of period change of several modes of KIC 8626021 are consistent with evolutionary cooling, but are not yet statistically significant. These modes offer the best possibility of measuring the neutrino production rate in a white dwarf. We also observe periodic and secular variations in the frequency of a combination mode that exactly matches the variations predicted by the parent modes, strong observational evidence that combination modes are created by the convection zone and are not normal modes. Periodic variations in the amplitudes of many of these modes is also noted. We hypothesize that these frequency variations are caused by complex variations of the magnetic field strength and geometry, analogous to behavior observed in the Sun.;In Part II we describe the MAESTRO software framework and the MAESTRO REDUCE algorithm. MAESTRO is a collection of astronomy specific MatLab software developed by the Whole Earth Telescope. REDUCE is an an algorithm that can extract the brightness of stars on a set of CCD images with minimal configuration and human interaction. The key to this algorithm is automatic identification of stars and a sophisticated implementation of geometric hashing.
机译:在第一部分中,我们报告了脉动DB白矮星EC 20058-5234和KIC 8626021以及脉动DB白矮星GD 66的正常模式频率的变化。EC 20058-5234和KIC 8626021的观测是由于GD 66的观测结果是基于白矮星脉动正时的行星搜索的一部分,它测量了白矮星的等离子体中微子产生速率。我们宣布发现多个正常模式频率的周期性和准周期性变化,这不可能归因于行星伴星的存在。我们注意到EC 20058-5234可能伴有行星伴星,并表明GD 66不能在几个AU轨道上将行星减至木星质量的一半。我们还宣布发现了所有三颗恒星的正常模态频率的长期变化,这些变化与单独的冷却是不一致的。重要的是,KIC 8626021的几种模式的周期变化率与演化冷却相一致,但尚无统计学意义。这些模式提供了测量白矮星中微子生产率的最佳可能性。我们还观察到组合模式频率的周期性和长期变化与母模式所预测的变化完全匹配,有力的观察证据表明组合模式是由对流带产生的,而不是正常模式。还注意到许多这些模式的振幅的周期性变化。我们假设这些频率变化是由磁场强度和几何形状的复杂变化引起的,类似于在太阳下观察到的行为。在第二部分中,我们描述了MAESTRO软件框架和MAESTRO REDUCE算法。 MAESTRO是全地望远镜开发的一组天文学专用MatLab软件。 REDUCE是一种算法,可以以最少的配置和人为干预提取一组CCD图像上星星的亮度。该算法的关键是恒星的自动识别和几何哈希的复杂实现。

著录项

  • 作者

    Dalessio, James Ruland.;

  • 作者单位

    University of Delaware.;

  • 授予单位 University of Delaware.;
  • 学科 Physics Astrophysics.;Physics General.;Physics Astronomy and Astrophysics.
  • 学位 Ph.D.
  • 年度 2013
  • 页码 228 p.
  • 总页数 228
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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