The formation, disruption and properties of pressure-supported stellar systems and implications for the astrophysics of galaxies [PDF]
Pavel Kroupa
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Doppler boosted dust emission and CIB-galaxy cross-correlations: a new probe of cosmology and astrophysics [PDF]
Abhishek S. Maniyar +2 more
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Galaxy clusters as astrophysical laboratories and probes of cosmology [PDF]
Galaxy clusters are the most recent of cosmological structures to have formed by the present time in the currently favoured hierarchical scenario of structure formation and are widely regarded as powerful probes of cosmology and galaxy formation physics alike.
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The Evolution of Galaxies and Their Environment [PDF]
The Third Teton Summer School on Astrophysics discussed the formation of galaxies, star formation in galaxies, galaxies and quasars at high red shift, and the intergalactic and intercluster medium and cooling flows.
Hollenbach, David +2 more
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Cosmology and astrophysics from relaxed galaxy clusters – II. Cosmological constraints [PDF]
A. Mantz +7 more
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Studying the evolution of large-scale structure with the VIMOS-VLT Deep Survey
The VIMOS-VLT Deep Survey (VVDS) currently offers a unique combination of depth, angular size and number of measured galaxies among surveys of the distant Universe: ~ 11,000 spectra over 0.5 deg2 to I_{AB}=24 (VVDS-Deep), 35,000 spectra over ~ 7 deg2 to ...
Bottini, D. +18 more
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"SZ spectroscopy" in the coming decade: Galaxy cluster cosmology and\n astrophysics in the submillimeter [PDF]
Kaustuv Basu +32 more
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The astrophysical behavior of open clusters along the Milky Way Galaxy
The main aim of this paper is to study the astrophysical behavior of open clusters' properties along the Milky Way Galaxy. Near-IR JHK (2MASS) photometry has been used for getting a homogeneous Catalog of 263 open clusters' parameters, which are studied for the first time by the author through the last five years.
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Astrocladistics: Multivariate Evolutionary Analysis in Astrophysics
The Hubble tuning fork diagram, based on morphology and established in the 1930s, has always been the preferred scheme for classification of galaxies. However, the current large amount of data up to higher and higher redshifts asks for more sophisticated
Fraix-Burnet, Didier
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Galaxy luminosity function pipeline for cosmology and astrophysics [PDF]
Nashwan Sabti +2 more
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