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GRB host galaxies studies with X-shooter†

机译:使用X-shooter †进行GRB宿主星系研究

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摘要

Gamma-ray bursts (GRBs) are the most powerful explosions since the formation of the Universe, associated with the death of massive stars or mergers of compact stellar objects. Several recent striking results strongly support the idea that host galaxies of GRBs are opening a new view on our understanding of galaxy formation and evolution, back to the very primordial universe at z ∼ 8. They form a unique sample of galaxies which cover a wide range of redshift, they are typically weak with low mass and unlike other methods they are not selected on luminosity. In recent years, thanks to the support of new generation instruments, multi-band photometry and spectroscopy allow us to better investigate the properties of these host galaxies (e.g., stellar mass, age, SFR, metallicity), to study their possible evolution and to compare them with field galaxies and other classes of galaxies. GRB host spectroscopy is one of the main science drivers behind the X-shooter spectrograph. In this paper, we present the first results of the program devoted to Italian-French GTO multiband spectroscopy of GRB host galaxies with X-shooter (© 2011 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)
机译:伽玛射线爆发(GRB)是自宇宙形成以来最强大的爆炸,与大质量恒星的死亡或紧凑型恒星物体的合并有关。最近的一些惊人结果有力地证明了GRB的宿主星系正在为我们对星系形成和演化的理解开辟新的视野,回到z〜8的原始宇宙。它们形成了一个涵盖范围广泛的独特星系样本。由于红移,它们通常质量较弱,质量较轻,并且与其他方法不同,它们不是根据亮度选择的。近年来,由于新一代仪器的支持,多波段光度法和光谱法使我们能够更好地研究这些宿主星系的特性(例如恒星质量,年龄,SFR,金属性),研究它们的可能演化并将它们与野外星系和其他类别的星系进行比较。 GRB主机光谱学是X-shooter光谱仪背后的主要科学驱动力之一。在本文中,我们介绍了该计划的第一个结果,该程序致力于使用X-shooter对GRB宿主星系进行意大利-法国GTO多波段光谱分析(©2011 WILEY-VCH Verlag GmbH&Co. KGaA,Weinheim)

著录项

  • 来源
    《Astronomische Nachrichten》 |2011年第3期|p.283-287|共5页
  • 作者单位

    INAF - Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monte Porzio Catone (RM), Italy;

    INAF - Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy;

    Dipartimento di Fisica, Università degli Studi Roma Tre, via della Vasca Navale 84, 00146 Roma, Italy;

    Max Planck Institute for Extraterrestrial Physics, 85748 Garching b. München, Germany;

    INAF - Istituto di Astrofísíca Spaziale e Físíca Cosmica, Sezione di Bologna, via Gobetti 101, 40129 Bologna, Italy;

    Laboratoire Galaxies Etoiles Physique et Instrumentation, Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon, France;

    INAF - Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy;

    Laboratoire Astroparticule et Cosmologie, 10 rue A. Domonet L. Duquet, 75205 Paris Cedex 13, France|DSM/IRFU/Service D'Astrophysique, CEA-Saclay, 91191 Gif-sur-Yvette, France;

    INAF - Osservatorio Astrofisico di Arcetri, INAF, Largo E. Fermi 5, 50125 Firenze, Italy;

    Laboratoire Galaxies Etoiles Physique et Instrumentation, Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon, France;

    INAF - Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 34143 Trieste, Italy|Scuola Normale Superiore, Piazza dei Cavalieri 7, 56126 Pisa, Italy|European Southern Observatory, Karl-Schwarzschild-Straße 2, 85748 Garching bei München, Germany;

    INAF - Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    galaxies: abundances; galaxies: formation; galaxies: evolution; gamma rays: bursts;

    机译:星系:丰度;星系:形成;星系:演化;伽玛射线:爆发;

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