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Recent progress in our knowledge of stellar populations in local dwarf spheroidal galaxies is briefly discussed. A few results are summarized including wide field observations of stellar populations and their spatial variations, studies of…

天体物理学 · 物理学 2009-11-11 Enrico V. Held

Some aspects of the chemical evolution of late-type dwarf galaxies are reviewed, together with their implications on three issues of cosmological relevance: similarity to primeval galaxies, derivation of the primordial helium abundance,…

天体物理学 · 物理学 2007-05-23 M. Tosi

What can we learn from the somewhat arduous study of old stellar populations in nearby galaxies? Unless the nearby universe is subtly anomalous, it should contain a relatively normal selection of galaxies whose histories are representative…

天体物理学 · 物理学 2009-10-31 Eline Tolstoy

The observable characteristics and subsequent evolution of young stellar populations is dominated by their massive stars. As our understanding of those massive stars and the factors affecting their evolution improves, so our interpretation…

星系天体物理 · 物理学 2022-09-28 Jan J. Eldridge , Elizabeth R. Stanway

I discuss the information provided by color-magnitude diagrams of different absolute magnitude limits in the study of the star formation histories of nearby galaxies. I review the recent progress made in the field, with emphasis on the…

天体物理学 · 物理学 2007-05-23 Carme Gallart

The stellar populations of galaxies contain a wealth of detailed information. From the youngest, most massive stars, to almost invisible remnants, the history of star formation is encoded in the stars that make up a galaxy. Extracting some,…

宇宙学与河外天体物理 · 物理学 2015-05-14 Jarle Brinchmann

Properties of nearby dwarf galaxies are briefly discussed. Dwarf galaxies vary widely in their star formation histories, the ages of their subpopulations, and in their enrichment history. Furthermore, many dwarf galaxies show evidence for…

天体物理学 · 物理学 2009-10-31 Eva K. Grebel

This review aims to give a summary of our understanding of galaxy evolution as infered from studies of nearby galaxies; how observations made with the Hubble Space Telescope have contributed significantly to our detailed understanding of…

天体物理学 · 物理学 2007-05-23 Eline Tolstoy

Within the Local Universe galaxies can be studied in great detail star by star, and here we review the results of quantitative studies in nearby dwarf galaxies. The Color-Magnitude Diagram synthesis method is well established as the most…

宇宙学与河外天体物理 · 物理学 2010-01-15 E. Tolstoy , V. Hill , M. Tosi

This review aims to give an overview of the contribution of the Hubble Space Telescope to our understanding of the detailed properties of Local Group dwarf galaxies and their older stellar populations. The exquisite stable high spatial…

天体物理学 · 物理学 2007-05-23 Eline Tolstoy

It is an obvious statement that all the galaxies we see today in and around our Local Group have been forming and evolving for a significant fraction of the age of the Universe. It is not a great leap of logic to further state that the…

天体物理学 · 物理学 2007-05-23 Eline Tolstoy

If we are to develop a comprehensive and predictive theory of galaxy formation and evolution, it is essential that we obtain an accurate assessment of how and when galaxies assemble their stellar populations, and how this assembly varies…

星系天体物理 · 物理学 2009-02-18 Thomas M. Brown , Marc Postman , Daniela Calzetti

The determination of stellar populations of galaxies are important for studying the formation and evolution of galaxies, because all galaxies contain many stars and they evolve with galaxies. Spectra data are usually used to determine the…

太阳与恒星天体物理 · 物理学 2013-02-04 Zhongmu Li

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

Stellar Populations are the fossil record of Galactic evolution. Interpretation of this record in the Local Group allows one to determine reliably the dominant physics controlling the evolution of those galaxies which are typical of the…

天体物理学 · 物理学 2007-05-23 Gerry Gilmore

The characteristics and properties of the stellar populations and evolutionary histories of Local Group galaxies are summarized and compared to predictions of cosmological models. No clear signature of the re-ionization epoch is observed;…

天体物理学 · 物理学 2009-11-13 Eva K. Grebel

We review current progress in the study of the stellar populations of early-type galaxies, both locally and at intermediate redshifts. In particular, we focus on the ages of these galaxies and their evolution in hopes of determining the…

天体物理学 · 物理学 2007-05-23 S. C. Trager , S. M. Faber , A. Dressler

I present a brief review of the stellar population properties of massive galaxies, focusing on early-type galaxies in particular, with emphasis on recent results from the ATLAS3D Survey. I discuss the occurrence of young stellar ages, cold…

宇宙学与河外天体物理 · 物理学 2015-06-12 Richard M. McDermid

The galaxies of the Local Group that are currently forming stars can serve as our laboratories for understanding star formation and the evolution of massive stars. In this talk I will summarize what I think we've learned about these topics…

天体物理学 · 物理学 2007-05-23 Philip Massey

The exploitation of the power and the spatial resolution of HST and new generation ground-based telescopes allows to measure with good precision the individual stars of galaxies in and beyond the Local Group. This leads to very successful…

天体物理学 · 物理学 2007-05-23 Monica Tosi
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