The top documents tagged [rich clusters]

Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL Revision Lecture
Documents Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL Revision Lecture

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Accelerating Growth Recipes, Ingredients and the Global Context Michael Spence The Israel 2021 Conference January 12-13, 2011
Documents Accelerating Growth Recipes, Ingredients and the Global Context Michael Spence The Israel 2021 Conference January 12-13, 2011

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Science at Q band SZ/CMB models: Q-band science Mark Birkinshaw University of Bristol
Documents Science at Q band SZ/CMB models: Q-band science Mark Birkinshaw University of Bristol

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How gallium nitride can save energy, purify water, be used in cancer therapy and improve our health!
Science How gallium nitride can save energy, purify water, be used in cancer therapy and improve our health!

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aa2838-05
Documents aa2838-05

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Stellar population results from NFPS: Age and Metallicity along the Red Sequence Russell Smith (Waterloo), Jenica Nelan (Dartmouth), Mike Hudson (Waterloo),
Documents Stellar population results from NFPS: Age and Metallicity along the Red Sequence Russell Smith (Waterloo), Jenica Nelan (Dartmouth), Mike Hudson (Waterloo),

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NEUTRAL HYDROGEN Frank Briggs RSAA and ATNF z = 8 z = 0
Documents NEUTRAL HYDROGEN Frank Briggs RSAA and ATNF z = 8 z = 0

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With a wide-field multi-IFU spectrograph. Clusters provide large samples of galaxies in a moderate field Unique perspective on the interaction of
Documents With a wide-field multi-IFU spectrograph. Clusters provide large samples of galaxies in a moderate field Unique perspective on the interaction of

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INFRARED-BRIGHT GALAXIES IN THE MILLENNIUM SIMULATION AND CMB CONTAMINATION DANIEL CHRIS OPOLOT DR. CATHERINE CRESS UWC
Documents INFRARED-BRIGHT GALAXIES IN THE MILLENNIUM SIMULATION AND CMB CONTAMINATION DANIEL CHRIS OPOLOT DR. CATHERINE CRESS UWC

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Fraction of galaxies of different types plotted as function of cluster radius and projected density Galaxy Morphology and Environment Main relation – E’s
Documents Fraction of galaxies of different types plotted as function of cluster radius and projected density Galaxy Morphology and Environment Main relation – E’s

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IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute
Documents IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute

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Susan CartwrightOur Evolving Universe1 Other galaxies n Telescopic images of the night sky reveal many other galaxies l l What do they look like? are
Documents Susan CartwrightOur Evolving Universe1 Other galaxies n Telescopic images of the night sky reveal many other galaxies l l What do they look like? are

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