arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 1102.0911astro-ph.CO
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利用超深光学图像研究早型星系的合并成因

Investigating the merger origin of Early-Type Galaxies using ultra-deep optical images

P. -A. Duc, J. -C. Cuillandre, K. Alatalo, L. Blitz, M. Bois, F. Bournaud, M. Bureau, M. Cappellari, P. Cote, R. L. Davies, T. A. Davis, P. T. de Zeeuw, E. Emse… 展开作者

P. -A. Duc, J. -C. Cuillandre, K. Alatalo, L. Blitz, M. Bois, F. Bournaud, M. Bureau, M. Cappellari, P. Cote, R. L. Davies, T. A. Davis, P. T. de Zeeuw, E. Emsellem, L. Ferrarese, E. Ferriere, S. Gwyn, S. Khochfar, D. Krajnovic, H. Kuntschner, P. -Y. Lablanche, L. MacArthur, R. M. McDermid, L. Michel-Dansac, R. Morganti, T. Naab, T. Oosterloo, M. Sarzi, N. Scott, P. Serra, A. Weijmans, L. M. Young

摘要:

星系的大规模聚集在其周围留下了各种印记,如壳,流和潮汐尾。这些精细结构的频率和性质取决于驱动质量组装的机制:例如,整体坍缩、快速冷气吸积,随后是剧烈的盘不稳定性、小合并或大的干/湿合并。因此,通过研究星系的外围,人们可以了解它们的主要形成机制。我在这里介绍我们正在进行的工作,以表征早期型Galerkin(ETGs),这是在低红移的星系的分级质量大会的强大的探针的郊区。这项工作依赖于在CFHT获得的超深光学图像,这些图像是作为Atlas-3D和NGVS项目的一部分获得的现场和集群ETG的宽视场MegaCam相机。最先进的数值模拟被用来解释数据。这些图像揭示了大量的未知的微弱结构,其微弱程度在g波段为29等角秒-2。这里给出了两个星系的初步结果。

英文摘要:

The mass assembly of galaxies leaves various imprints on their surroundings, such as shells, streams and tidal tails. The frequency and properties of these fine structures depend on the mechanism driving the mass assembly: e.g. a monolithic collapse, rapid cold-gas accretion followed by violent disk instabilities, minor mergers or major dry / wet mergers. Therefore, by studying the outskirts of galaxies, one can learn about their main formation mechanism. I present here our on-going work to characterize the outskirts of Early-Type Galaxies (ETGs), which are powerful probes at low redshift of the hierarchical mass assembly of galaxies. This work relies on ultra-deep optical images obtained at CFHT with the wide-field of view MegaCam camera of field and cluster ETGs obtained as part of the Atlas-3D and NGVS projects. State of the art numerical simulations are used to interpret the data. The images reveal a wealth of unknown faint structures at levels as faint as 29 mag arcsec-2 in the g-band. Initial results for two galaxies are presented here.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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