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We summarize recent advances in the determination of the cosmic history of star formation and other properties of high-z galaxies, and the relevance of this information in our understanding of the formation of structures. We emphasize the…

天体物理学 · 物理学 2016-01-27 Gian Luigi Granato , Laura Silva

Interstellar dust is a key physical ingredient of galaxies, obscuring star formation, regulating the heating and cooling of the gas, and building-up chemical complexity. In this manuscript, I give a wide review of interstellar dust…

星系天体物理 · 物理学 2022-02-07 Frédéric Galliano

Dust-obscured star formation has dominated the cosmic history of star formation since z = 4. However, the recent finding of significant amount of dust in galaxies out to z = 8 has opened the new frontier of investigating the origin of dust…

星系天体物理 · 物理学 2024-02-01 Raffaella Schneider , Roberto Maiolino

I review a technique for interpreting faint galaxy data which traces the evolution with cosmic time of the galaxy luminosity density, as determined from several deep spectroscopic samples and the HDF. The method relies on the rest frame UV…

天体物理学 · 物理学 2007-05-23 Piero Madau

This paper reviews the dust content of the high redshift (z > 2) universe. Studies of the various "species" in the high-z "zoo" show that almost all have strong evidence for containing dust. The one exception, where the evidence is not yet…

天体物理学 · 物理学 2007-05-23 G. R. Meurer

The study of high-redshift objects is rapidly developing, allowing to build the star formation history of the Universe. Since most of the flux from starbursts comes out in the FIR region, the submm and mm are privileged domains for the…

天体物理学 · 物理学 2009-10-31 F. Combes

We discuss recent advances in the study of dusty, massive galaxies at z>1 arising from the first extensive spectroscopic surveys.

天体物理学 · 物理学 2007-05-23 Ian Smail , Scott Chapman , Andrew Blain , Rob Ivison

Observations of quasar absorption systems relevant for studies of star formation at redshift 2 </= z </= 4 are briefly reviewed. Emphasis is given on the role played by dust in our understanding of the star formation history of galaxies…

天体物理学 · 物理学 2007-12-11 Juan Vladilo

It is well established in the local Universe that regions of high star-formation rate are dusty. As a result of this physical causal link, galaxies of increasing current star formation activity emit a larger proportion of their bolometric…

天体物理学 · 物理学 2007-05-23 Matthew A. Malkan

In the current era of high-z galaxy discovery with JWST and ALMA, our ability to study the stellar populations and ISM conditions in a diverse range of galaxies at Cosmic Dawn has rapidly improved. At the same time, the need to understand…

星系天体物理 · 物理学 2024-03-05 Sidney Lower , Desika Narayanan , Chia-Yu Hu , George C. Privon

The generation and evolution of dust in galaxies are important tracers for star formation, and can characterize the rest-frame ultraviolet to infrared emission from the galaxies. In particular understanding dust in high-redshift galaxies…

星系天体物理 · 物理学 2023-10-05 Daichi Tsuna , Yurina Nakazato , Tilman Hartwig

Dust plays an important role in the evolution of a galaxy, since it is one of the main ingredients for efficient star formation. Dust grains are also a sink/source of metals when they are created/destroyed, and, therefore, a self-consistent…

星系天体物理 · 物理学 2020-04-08 I. Millán-Irigoyen , M. Mollá , Y. Ascasibar

In these lectures I review observations of star-forming molecular clouds in our Galaxy and nearby galaxies to develop a physical intuition for understanding star formation in the local and high-redshift Universe. A lot of this material is…

宇宙学与河外天体物理 · 物理学 2012-11-05 Nick Z. Scoville

This article gives an overview of the constitution, physical conditions and observables of dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial distribution of dust in these objects, and its…

星系天体物理 · 物理学 2022-08-10 F. Galliano , M. Galametz , A. P. Jones

This article is based on an invited talk given by V. P. Kulkarni at the 8th Cosmic Dust meeting. Dust has a profound effect on the physics and chemistry of the interstellar gas in galaxies and on the appearance of galaxies. Understanding…

星系天体物理 · 物理学 2016-12-07 Varsha P. Kulkarni , Monique C. Aller , Donald G. York , Daniel E. Welty , Giovanni Vladilo , Debopam Som

This review describes where we are today in light of the dust and gas properties and their relation to star formation, in low metallicity galaxies of the local universe following recent surveys from sensitive infrared space telescopes,…

星系天体物理 · 物理学 2019-11-06 Suzanne C. Madden , Diane Cormier

Dust grains play a fundamental role in galaxies, influencing both their evolution and observability. As a result, incorporating dust physics into galaxy evolution simulations is essential. This is a challenging task due to the finite…

星系天体物理 · 物理学 2025-04-16 Massimiliano Parente

The recent detection of the Cosmic Infrared Background in FIRAS and DIRBE residuals, and the observations of IR/submm sources by the ISOPHOT and SCUBA instruments have shed new light on the optically dark side of galaxy formation. It turns…

天体物理学 · 物理学 2007-05-23 B. Guiderdoni

The past century of interstellar dust has brought us from first ignoring it to finding that it is an important component of the interstellar medium and plays an important role in the evolution of galaxies, the formation of stars and…

天体物理学 · 物理学 2007-05-23 Aigen Li , J. Mayo Greenberg

Galactic interstellar dust has a profound impact not only on our observations of objects throughout the Universe, but also on the morphology, star formation, and chemical evolution of the Galaxy. The advent of massive imaging and…

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