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首页> 外文期刊>Astronomy and astrophysics >The VIMOS Public Extragalactic Redshift Survey (VIPERS) - Downsizing of the blue cloud and the influence of galaxy size on mass quenching over the last eight billion years
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) - Downsizing of the blue cloud and the influence of galaxy size on mass quenching over the last eight billion years

机译:VIMOS公共河外红移调查(VIPERS)-过去80亿年中蓝云的缩小以及星系大小对质量猝灭的影响

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摘要

We use the full VIPERS redshift survey in combination with SDSS-DR7 to explore the relationships between star-formation history (using d4000), stellar mass and galaxy structure, and how these relationships have evolved since z ~ 1 . We trace the extents and evolutions of both the blue cloud and red sequence by fitting double Gaussians to the d4000 distribution of galaxies in narrow stellar mass bins, for four redshift intervals over 0 & z & 1 . This reveals downsizing in star formation, since the high-mass limit of the blue cloud has retreated steadily with time from ? ~ 10~(11.2 ) M _(⊙) at z ~ 0.9 to ? ~ 10~(10.7 ) M _(⊙) by the present day. The number density of massive blue-cloud galaxies ( ? & 10~(11) M _(⊙) , d 4000 & 1.55 ) drops sharply by a factor five between z ~ 0.8 and z ~ 0.5 . These galaxies are becoming quiescent at a rate that largely matches the increase in the numbers of massive passive galaxies seen over this period. We examine the size-mass relation of blue-cloud galaxies, finding that its high-mass boundary runs along lines of constant ? / r _(e) or equivalently inferred velocity dispersion. Larger galaxies can continue to form stars to higher stellar masses than smaller galaxies. As blue-cloud galaxies approach this high-mass limit, entering a narrow diagonal region within the size-mass plane termed the “quenching zone”, they start to be quenched, their d4000 values increasing to push them towards the green valley. In parallel, their structures change, showing higher Sérsic indices and central stellar mass densities. For these galaxies, bulge growth is required for them to reach the high-mass limit of the blue cloud and be quenched by internal mechanisms. The blue-cloud galaxies that are being quenched at z ~ 0.8 lie along the same size-mass relation as present day quiescent galaxies and seem the likely progenitors of today’s S0s.
机译:我们将完整的VIPERS红移调查与SDSS-DR7结合使用,以探索恒星形成历史(使用d4000),恒星质量和星系结构之间的关系,以及自z〜1以来这些关系如何演变。通过使双高斯拟合到狭窄恒星质量仓中的d4000分布的星系,在0≤0的四个红移间隔内,我们追踪了蓝云和红色序列的程度和演化。 & 1。这揭示了恒星形成的缩减,因为随着时间的推移,蓝云的高质量极限已随着时间稳定地减小。 z〜0.9时的〜10〜(11.2)M _(⊙)到今天为止〜10〜(10.7)M _(⊙)。块状大的蓝云星系的数密度(?> 10〜(11)M _(⊙),d 4000 <1.55)急剧下降了五倍,介于z〜0.8和z〜0.5之间。这些星系正以与在此期间看到的大规模被动星系数量增加基本匹配的速率变得静止。我们检查了蓝云星系的大小质量关系,发现其高质量边界沿常数? / r _(e)或等效推论的速度色散。与较小的星系相比,较大的星系可以继续形成更高质量的恒星。当蓝云星系接近这个高质量极限时,进入质量块平面内称为“淬火区”的狭窄对角线区域,它们开始被淬灭,其d4000值增加,将其推向绿色山谷。同时,它们的结构发生变化,显示出更高的Sérsic指数和中心恒星质量密度。对于这些星系,需要凸起增长才能达到蓝云的高质量极限并通过内部机制将其猝灭。在z〜0.8处被淬灭的蓝云星系与当今的静态星系具有相同的大小质量关系,并且似乎是当今S0的祖先。

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