Properties of thick discs formed in clumpy galaxies
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/441/1/243/3016817/stu544.pdf
Reference143 articles.
1. Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. II. The Fine Structure of Simulated Galactic Disks
2. Disc formation and the origin of clumpy galaxies at high redshift
3. TOWARD A COMPLETE ACCOUNTING OF ENERGY AND MOMENTUM FROM STELLAR FEEDBACK IN GALAXY FORMATION SIMULATIONS
4. A Spectroscopic Study of the Ancient Milky Way: F‐ and G‐Type Stars in the Third Data Release of the Sloan Digital Sky Survey
5. A FIRST CONSTRAINT ON THE THICK DISK SCALE LENGTH: DIFFERENTIAL RADIAL ABUNDANCES IN K GIANTS AT GALACTOCENTRIC RADII 4, 8, AND 12 kpc
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2. Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 Using the Galaxy Zoo;The Astrophysical Journal;2021-05-01
3. Clumpy galaxies in cosmological simulations: the effect of ISM model;Monthly Notices of the Royal Astronomical Society;2019-07-30
4. A Tale of Two Clump Masses: A new way to study clump formation in simulations;Monthly Notices of the Royal Astronomical Society;2019-04-27
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