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相关论文: Massive Stars in the Local Group: Star Formation a…

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In this contribution I present the main research activities of the IAC ``Stellar Populations in Galaxies'' research Group, with emphasis on the subtopics directly related with the study of the evolution of nearby galaxies. In particular, I…

天体物理学 · 物理学 2007-05-23 Carme Gallart

Observations of star-forming galaxies in the distant Universe have confirmed the importance of massive stars in shaping galaxy emission and evolution. Distant stellar populations are unresolved, and the limited data available must be…

星系天体物理 · 物理学 2020-06-10 E R Stanway , J J Eldridge

Galaxies represent the visible fabric of the Universe and there has been considerable progress recently in both observational and theoretical studies. The underlying goal is to understand the present-day diversity of galaxy forms, masses…

天体物理学 · 物理学 2007-05-23 Richard Ellis

In the present-day universe, it appears that most, and perhaps all, massive stars are born in star clusters. It also appears that all star clusters contain stars drawn from an approximately universal initial mass function, so that almost…

天体物理学 · 物理学 2017-03-08 Jonathan C. Tan

Extreme star formation includes star formation in starbursts and regions forming super star clusters. We survey the current problems in our understanding of the star formation process in starbursts and super star clusters - initial mass…

星系天体物理 · 物理学 2010-09-09 Jean L. Turner

This review focuses on how galaxies and their globular cluster systems form. I first discuss the now fairly convincing evidence that some globular clusters form in galaxy starbursts/mergers. One way these observations are valuable is they…

天体物理学 · 物理学 2007-05-23 Stephen E. Zepf

The current status of carbon stars in the Local Group and beyond, is discussed. Although many carbon stars and late M-stars have been identified in Local Group galaxies, a coherent understanding in terms of the chemical evolution- and star…

天体物理学 · 物理学 2007-05-23 M. A. T. Groenewegen

The history of the formation and evolution of the Milky Way Galaxy is found in the spatial distribution, kinematics, age and chemical abundance distributions of long-lived stars. From this fossil record one can in principle extract the star…

天体物理学 · 物理学 2016-08-30 Rosemary F. G. Wyse , Gerard Gilmore

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 evolution of galaxies results from a combination of internal and external processes. The star formation is an internal process transforming cold and dense cores of molecular clouds to stars. It may be triggered internally by expanding…

天体物理学 · 物理学 2008-11-26 Jan Palouš

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 ensemble of all star clusters in a galaxy constitutes its star cluster system. In this review, the focus of the discussion is on the ability of star clusters, particularly the systems of old massive globular clusters (GCSs), to mark the…

星系天体物理 · 物理学 2015-05-14 William E. Harris

Spiral galaxies offer a unique opportunity to study the role of star formation in galaxy evolution and to test various theoretical star formation schemes. I review some recent relevant work on the evolution of spiral galaxies. Detailed…

天体物理学 · 物理学 2007-05-23 Nikos Prantzos

The goal of this investigation is to reconstruct the cosmic star formation rate density history from local observations and in doing so to gain insight into how galaxies might have formed and evolved. A new chemical evolution model is…

天体物理学 · 物理学 2009-11-10 F. D. A. Hartwick

The combination of huge databases of galaxy spectra and advances in evolutionary synthesis models in the past few years has renewed interest in an old question: How to estimate the star formation history of a galaxy out of its integrated…

天体物理学 · 物理学 2009-11-13 Roberto Cid Fernandes

I review recent observational progress concerning the evolution of the morphological distribution of galaxies in the rich cluster environment and in the faint field population. By coupling HST imagery with ground-based spectroscopic…

天体物理学 · 物理学 2007-05-23 Richard S Ellis

Our current knowledge of carbon stars in the Local Group and beyond, is discussed. Although many carbon stars and late M-stars have been identified in external galaxies a coherent understanding in terms of the chemical evolution- and star…

天体物理学 · 物理学 2007-05-23 M. A. T. Groenewegen

The formation and evolution of galaxies is one of the great outstanding problems of astrophysics. Within the broad context of hierachical structure formation, we have only a crude picture of how galaxies like our own came into existence. A…

天体物理学 · 物理学 2011-03-10 Ken Freeman , Joss Bland-Hawthorn

One of the challenges for stellar astrophysics is to reach the point at which we can undertake reliable spectral synthesis of unresolved populations in young, star-forming galaxies at high redshift. Here I summarise recent studies of…

宇宙学与河外天体物理 · 物理学 2015-05-20 C. J. Evans

Massive galaxies, such as nearby ellipticals, have relatively low number densities, yet they host the majority of the stellar mass in the universe. Understanding their origin is a central problem of galaxy formation. Age dating of stellar…

天体物理学 · 物理学 2007-05-23 Christopher J. Conselice