Ram pressure stripping of disk galaxies - From high to low density environments
A&A, 433 3 (2005) 875-895
Published online: 2005-03-29
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ABUNDANT MOLECULAR GAS AND INEFFICIENT STAR FORMATION IN INTRACLUSTER REGIONS: RAM PRESSURE STRIPPED TAIL OF THE NORMA GALAXY ESO137-001
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Cold gas properties of theHerschelReference Survey
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Direct Simulation Monte Carlo for astrophysical flows – II. Ram-pressure dynamics
Martin D. WeinbergMonthly Notices of the Royal Astronomical Society 438 (4) 3007 (2014)
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On the origin of the faint-end of the red sequence in high-density environments
Alessandro Boselli and Giuseppe GavazziThe Astronomy and Astrophysics Review 22 (1) (2014)
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The Herschel Virgo Cluster Survey – XIV. Transition-type dwarf galaxies in the Virgo cluster
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LoCuSS: THE STEADY DECLINE AND SLOW QUENCHING OF STAR FORMATION IN CLUSTER GALAXIES OVER THE LAST FOUR BILLION YEARS
C. P. Haines, M. J. Pereira, G. P. Smith, et al.The Astrophysical Journal 775 (2) 126 (2013)
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Unveiling the corona of the Milky Way via ram-pressure stripping of dwarf satellites
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P. Merluzzi, G. Busarello, M. A. Dopita, et al.Monthly Notices of the Royal Astronomical Society 429 (2) 1747 (2013)
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THE NARROW X-RAY TAIL AND DOUBLE Hα TAILS OF ESO 137-002 IN A3627
B. Zhang, M. Sun, L. Ji, et al.The Astrophysical Journal 777 (2) 122 (2013)
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Planets, Stars and Stellar Systems
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