Titlebook: Outskirts of Galaxies; Johan H. Knapen,Janice C. Lee,Armando Gil de Paz Book 2017 Springer International Publishing AG 2017 Galaxies struc

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改變

Resolved Stellar Populations as Tracers of Outskirts,tous and to be (at least in part) the product of past merger and/or accretion events. The advent of wide-field surveys in the last two decades has revolutionized our view of our own Galaxy and its closest “sister”, Andromeda, revealing copious tidal streams from past and ongoing accretion episodes,

STRIA

textile

Communicate

Nebulizer

Molecular Gas in the Outskirts,their relationship with star formation and galaxy evolution. We review the basic equations that are used in normal environments to estimate physical parameters like the molecular gas mass from CO line emission and dust continuum emission. Then we discuss how those estimates may be affected when appl

maculated

H, in the Outskirts of Nearby Galaxies,al resolution H. imaging, the contribution it made to the dark matter problem, and the current tension between several dynamical methods to break the disk-halo degeneracy. I then turn to the flaring problem, which could in principle probe the shape of the dark halo. Instead, however, a lot of attent

GREG

Ultra-Deep Imaging: Structure of Disks and Haloes, disks and haloes, highlighting the technical advances as well as the challenges and summarizing observational results in the context of modern theory and simulations. The deepest modern galaxy imaging comes from three main sources: (1) surveys such as the Sloan Digital Sky Survey’s Stripe?82 projec

Interregnum

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