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相关论文: Star Formation in the Milky Way and Nearby Galaxie…

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I present a brief review of some of the most recent and active topics of star formation process in the Milky Way using mid and far infrared observations, and motivated by the research being carried out by our science group using data…

星系天体物理 · 物理学 2015-06-12 A. Noriega-Crespo

I review observational studies of the large-scale star formation process in nearby galaxies. A wealth of new multi-wavelength data provide an unprecedented view on the interplay of the interstellar medium and (young) stellar populations on…

星系天体物理 · 物理学 2015-06-11 Andreas Schruba

The relations between star formation and properties of molecular clouds are studied based on a sample of star forming regions in the Galactic Plane. Sources were selected by having radio recombination lines to provide identification of…

太阳与恒星天体物理 · 物理学 2017-03-08 Nalin Vutisalchavakul , Neal J. Evans , Mark Heyer

Studies of molecular clouds and young stars near the sun have provided invaluable insights into the process of star formation. Indeed, much of our physical understanding of this topic has been derived from such studies. Perhaps the two most…

星系天体物理 · 物理学 2016-02-03 Charles J. Lada

Star formation takes place in the dense gas phase, and therefore a simple dense gas and star formation rate relation has been proposed. With the advent of multi-beam receivers, new observations show that the deviation from linear relations…

星系天体物理 · 物理学 2020-02-19 Quang Nguyen-Luong , Neal Evans , Kee-Tae Kim , Hyunwoo Kang , DEGAMA survey members

The processes regulating star formation in galaxies are thought to act across a hierarchy of spatial scales. To connect extragalactic star formation relations from global and kpc-scale measurements to recent cloud-scale resolution studies,…

Observations of the interstellar medium are key to deciphering the physical processes regulating star formation in galaxies. However, observational uncertainties and detection limits can bias the interpretation unless carefully modeled.…

星系天体物理 · 物理学 2020-12-14 Robert Feldmann

The conversion of gas into stars is a fundamental process in astrophysics and cosmology. Stars are known to form from the gravitational collapse of dense clumps in interstellar molecular clouds, and it has been proposed that the resulting…

Giant molecular clouds (GMCs) are the primary reservoirs of cold, star-forming molecular gas in the Milky Way and similar galaxies, and thus any understanding of star formation must encompass a model for GMC formation, evolution, and…

The star-formation histories of the main stellar components of the Milky Way constrain critical aspects of galaxy formation and evolution. I discuss recent determinations of such histories, together with their interpretation in terms of…

星系天体物理 · 物理学 2015-05-13 Rosemary F. G. Wyse

The chemical abundances in the atmosphere of a star provide unique information about the gas from which that star formed, and, modulo processes that are not important for the vast majority of stars, such as mass transfer in close binary…

星系天体物理 · 物理学 2015-05-14 Rosemary F. G. Wyse

We present a review of recent studies of the formation and evolution of the Milky Way galaxy, in particular based on large samples of non-kinematically selected stars with available proper motions. The Milky Way is argued to be a reasonable…

天体物理学 · 物理学 2007-05-23 Timothy C. Beers , Masashi Chiba

The inner few hundred parsecs of the Milky Way harbours gas densities, pressures, velocity dispersions, an interstellar radiation field and a cosmic ray ionisation rate orders of magnitude higher than the disc; akin to the environment found…

星系天体物理 · 物理学 2017-06-21 A. T. Barnes , S. N. Longmore , C. Battersby , J. Bally , J. M. D. Kruijssen , J. D. Henshaw , D. L. Walker

Quantification of the Galaxy's star formation history involves both the duration and the rate of formation, with these parameters being known with different precision for different populations. The early rate of star formation is knowable…

天体物理学 · 物理学 2007-05-23 Gerry Gilmore

This review examines the state-of-the-art knowledge of high-mass star and massive cluster formation, gained from ambitious observational surveys, which acknowledge the multi-scale characteristics of these processes. After a brief overview…

星系天体物理 · 物理学 2018-03-19 Frederique Motte , Sylvain Bontemps , Fabien Louvet

The formation of stars is a key process in astrophysics. Detailed knowledge of the physical mechanisms that govern stellar birth is a prerequisite for understanding the formation and evolution of our galactic home, the Milky Way. A theory…

星系天体物理 · 物理学 2012-02-07 Ralf S. Klessen , Mark R. Krumholz , Fabian Heitsch

We review the evidence for a constant star formation rate per unit mass in dense molecular gas in the Milky Way and the extragalactic correlations of L_IR with L' from observations of dense molecular gas. We discuss the connection between…

天体物理学 · 物理学 2007-11-30 Yancy L. Shirley , Jingwen Wu , R. Shane Bussmann , Al Wootten

In this paper we investigate scaling relations between star formation rates and molecular gas masses for both local Galactic clouds and a sample of external galaxies. We specifically consider relations between the star formation rates and…

星系天体物理 · 物理学 2015-06-03 Charles J. Lada , Jan Forbrich , Marco Lombardi , Joao F. Alves

This paper discusses how cosmic gas accretion controls star formation, and summarizes the physical properties expected for the cosmic gas accreted by galaxies. The paper also collects observational evidence for gas accretion sustaining star…

星系天体物理 · 物理学 2015-06-19 J. Sanchez Almeida , B. G. Elmegreen , C. Munoz-Tunon , D. M. Elmegreen

In this review I will describe a number of recent advances in extragalactic astronomy. First of all I will describe our current best estimates of the star formation history of the Universe. Then I will describe measurements of local…

天体物理学 · 物理学 2007-05-23 Neil Trentham
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