Primordial star clusters at extreme magnification

Erik Zackrisson*, Juan González, Simon Eriksson, Saghar Asadi, Chalence Safranek-Shrader, Michele Trenti, Akio K. Inoue

*この研究の対応する著者

研究成果: Article査読

20 被引用数 (Scopus)

抄録

Gravitationally lensed galaxies with magnification μ ≈ 10-100 are routinely detected at high redshifts, but magnifications significantly higher than this are hampered by a combination of low probability and large source sizes. Magnifications of μ ~ 1000 may none the less be relevant in the case of intrinsically small, high-redshift objects with very high number densities. Here, we explore the prospects of detecting compact (≲10 pc), high-redshift (z ≳ 7) Population III star clusters at such extreme magnifications in large-area surveys with planned telescopes like Euclid, Wide Field Infrared Survey Telescope and Wide-field Imaging Surveyor for High-redshift (WISH). We find that the planned WISH 100 deg2 ultradeep survey may be able to detect a small number of such objects, provided that the total stellar mass of these star clusters is ≳104M. If candidates for such lensed Population III star clusters are found, follow-up spectroscopy of the surrounding nebula with the James Webb Space Telescope or ground-based Extremely Large Telescopes should be able to confirm the Population III nature of these objects. Multiband photometry of these objects with the James Webb Space Telescope also has the potential to confirm that the stellar initial mass function in these Population III star clusters is top-heavy, as supported by current simulations.

本文言語English
ページ(範囲)3057-3063
ページ数7
ジャーナルMonthly Notices of the Royal Astronomical Society
449
3
DOI
出版ステータスPublished - 2015 5月 21
外部発表はい

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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