Grain Nucleation Experiments and other Laboratory Data: Why Galaxies Care About AGB Stars II: Shining Exammples and Common Inhabitants,

Research output: Other contribution › Research

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Grain Nucleation Experiments and other Laboratory Data : Why Galaxies Care About AGB Stars II: Shining Exammples and Common Inhabitants, . / Andersen, Anja C.

16-20/8-2010, Vienna, University Campus, Austria. 2010, Invited talks.

Research output: Other contribution › Research

Harvard

Andersen, AC 2010, Grain Nucleation Experiments and other Laboratory Data: Why Galaxies Care About AGB Stars II: Shining Exammples and Common Inhabitants, . 16-20/8-2010, Vienna, University Campus, Austria.

APA

Andersen, A. C. (2010, Aug 18). Grain Nucleation Experiments and other Laboratory Data: Why Galaxies Care About AGB Stars II: Shining Exammples and Common Inhabitants, .

Vancouver

Andersen AC. Grain Nucleation Experiments and other Laboratory Data: Why Galaxies Care About AGB Stars II: Shining Exammples and Common Inhabitants, . 2010.

Author

Andersen, Anja C. / Grain Nucleation Experiments and other Laboratory Data : Why Galaxies Care About AGB Stars II: Shining Exammples and Common Inhabitants, . 2010. 16-20/8-2010, Vienna, University Campus, Austria.

Bibtex

@misc{d21c2bc8b10642afbeff4307ed017e57,
title = "Grain Nucleation Experiments and other Laboratory Data: Why Galaxies Care About AGB Stars II: Shining Exammples and Common Inhabitants, ",
abstract = "Stars are conspicuous components of galaxies, and the sites of the creation of most chemical elements. Due to their brightness and their production of heavy elements, stars on the Asymptotic Giant Branch (AGB) play an important role for understanding stellar and galactic evolution. This conference aims to build a bridge between AGB research and its application to the modelling of stellar populations and the chemical evolution of galaxies. Current developments and challenges on both sides will be discussed to reach an understanding of possibilities, limitations, and needs in both areas, and hence to improve our knowledge about the role of AGB stars in the context of galaxies. This is the follow-up meeting to the Vienna conference on a similar topic in August 2006 (Link). This time the focus of the meeting will be: Complex Atmospheres & Interiors: Dynamics, Evolution & Abundances Environment: Mass Loss, Chemistry & Geometry Common Inhabitants: Population Studies & Synthesis Models Out There: Magellanic Clouds, Local Group & Beyond Perspectives Near and Far: ALMA, Herschel, JWST, ELTs, ... ",
author = "Andersen, {Anja C.}",
year = "2010",
month = aug,
day = "18",
language = "English",
type = "Other",

}

RIS

TY - GEN

T1 - Grain Nucleation Experiments and other Laboratory Data

T2 - Why Galaxies Care About AGB Stars II: Shining Exammples and Common Inhabitants,

AU - Andersen, Anja C.

PY - 2010/8/18

Y1 - 2010/8/18

N2 - Stars are conspicuous components of galaxies, and the sites of the creation of most chemical elements. Due to their brightness and their production of heavy elements, stars on the Asymptotic Giant Branch (AGB) play an important role for understanding stellar and galactic evolution. This conference aims to build a bridge between AGB research and its application to the modelling of stellar populations and the chemical evolution of galaxies. Current developments and challenges on both sides will be discussed to reach an understanding of possibilities, limitations, and needs in both areas, and hence to improve our knowledge about the role of AGB stars in the context of galaxies. This is the follow-up meeting to the Vienna conference on a similar topic in August 2006 (Link). This time the focus of the meeting will be: Complex Atmospheres & Interiors: Dynamics, Evolution & Abundances Environment: Mass Loss, Chemistry & Geometry Common Inhabitants: Population Studies & Synthesis Models Out There: Magellanic Clouds, Local Group & Beyond Perspectives Near and Far: ALMA, Herschel, JWST, ELTs, ...

AB - Stars are conspicuous components of galaxies, and the sites of the creation of most chemical elements. Due to their brightness and their production of heavy elements, stars on the Asymptotic Giant Branch (AGB) play an important role for understanding stellar and galactic evolution. This conference aims to build a bridge between AGB research and its application to the modelling of stellar populations and the chemical evolution of galaxies. Current developments and challenges on both sides will be discussed to reach an understanding of possibilities, limitations, and needs in both areas, and hence to improve our knowledge about the role of AGB stars in the context of galaxies. This is the follow-up meeting to the Vienna conference on a similar topic in August 2006 (Link). This time the focus of the meeting will be: Complex Atmospheres & Interiors: Dynamics, Evolution & Abundances Environment: Mass Loss, Chemistry & Geometry Common Inhabitants: Population Studies & Synthesis Models Out There: Magellanic Clouds, Local Group & Beyond Perspectives Near and Far: ALMA, Herschel, JWST, ELTs, ...

M3 - Other contribution

CY - 16-20/8-2010, Vienna, University Campus, Austria

ER -

ID: 33537253