On the Origin (and Evolution) of Baryonic Galaxy Halos

doi:10.3390/books978-3-03842-721-6

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Paperback

Keywords

galaxies; formation; evolution; halos; galaxy formation and evolution; integral field unit spectroscopy; cD galaxies; galaxies: formation; galaxies: evolution; galaxies: elliptical and lenticular; galaxies; formation; evolution; halos; interstellar matter; stellar evolution; galactic halo; galaxies: elliptical and lenticular, cD; galaxies: halos; galaxies: individual (NGC 3923); galaxies: structure; galaxies: star clusters: general; elliptical galaxies; globular clusters; evolution; techniques: image processing; galaxies: elliptical and lenticular, cD; galaxies: fundamental parameters; galaxies: formation; galaxies: halos; galaxy formation and evolution; stellar halo; numerical simulations; globular clusters; star formation; abundances; stellar halos; cosmology: theory; galaxies: evolution; galaxies: interactions; galaxies: kinematics and dynamics; galaxies: structure; methods: numerical; stellar shells; stellar metallicities; galaxy clusters; intracluster medium; galaxies; stellar population; numerical simulation; globular cluster; lenticular galaxies; galaxy halos; early-type galaxies; globular cluster; galaxy halos; elliptical galaxies; globular clusters; galaxy haloes; galaxies: evolution; galaxies: groups; galaxies: halos; galaxies: photometry; kinematically distinct cores; galaxy merger; numerical simulation; galaxy formation; galaxies: star clusters: general; galaxies: halos; galaxies: elliptical and lenticular; CD; galaxy: kinematics and dynamics; galaxy: halo; galaxy: abundances; galaxy: structure; galaxy: formation; cosmology: dark matter; methods: statistical; methods: numerical; galaxies: galaxy formation; galactic disks; stellar halos; Milky Way; 21-cm emission line; Galaxy halo; interstellar medium; galaxies: abundances; galaxies: star clusters; globular clusters: general; galaxies: elliptical and lenticular, cD; galaxies: evolution; galaxies: star clusters: individual: NGC 3258 & NGC 3268; galaxy clusters; intracluster light; numerical simulation; spiral galaxies; dust mass; dust-to-gas ratio; nearby galaxies; magnetic fields; molecules; galaxies: evolution; galaxies: halos; galaxies: individual (M31); galaxies: elliptical and lenticular; cD–X-rays: galaxies; galaxies: general; galaxies: evolution; galaxies: halos; galaxies: stellar content; galaxies: bulges; galaxies: merger history

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On the Origin (and Evolution) of Baryonic Galaxy Halos

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February 2018

230 pages

ISBN 978-3-03842-722-3 (Paperback)
ISBN 978-3-03842-721-6 (PDF)

https://doi.org/10.3390/books978-3-03842-721-6

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This is a Reprint of the Special Issue On the Origin (and Evolution) of Baryonic Galaxy Halos that was published in

Physical Sciences

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On the Origin (and Evolution) of Baryonic Galaxy Halos

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