Difference between revisions of "StarFormationInMW"
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===Star Formation History Links=== | ===Star Formation History Links=== | ||
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| + | [http://www.ifa.hawaii.edu/~ger/ASTRO-110_sp08/Lecture23_The%20Galaxy.pdf Contains an overview of a number of item, including the stars, gas, dust cycle] | ||
[http://arxiv.org/pdf/0907.0415v1.pdf One review of the star formation history (very technical)] | [http://arxiv.org/pdf/0907.0415v1.pdf One review of the star formation history (very technical)] | ||
Revision as of 19:57, 31 January 2013
Star formation has been ongoing in the Milky Way for most of its life (>10 Billion years). Present day star formation occurs in the disk of the Milky Way, with some recent evidence of ongoing activity in the central part of the Galaxy.
As stars form, age, evolve they bring fundamental changes in the composition and structure of the Galaxy. The star formation process exhausts the local gas and dust, turning it into stars. For the most part, the gas and dust is effectively "locked" into low mass stars which continue to exist for Billions of years, or cool off as low-mass brown dwarfs for eternity. Higher mass objects re-release some of the gas and dust in ejecta, winds or supernovae.
Star Formation History Links
Contains an overview of a number of item, including the stars, gas, dust cycle One review of the star formation history (very technical)
Learning Points
- What is Metallicity? What does it tell us?
- Where are the old stars in the Milky Way?
- Where are the youngest stars in the Milky Way?
