Mass loss from dwarf spheroidal galaxies: the origins of shallow dark matter cores and exponential surface brightness profiles

Overview of attention for article published in Monthly Notices of the Royal Astronomical Society, January 2005

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@GalacticRAVE @JossBlandHawtho However, repeated inflow/outflow can work if star formation proceeds in multiple bursts (https://t.co/wfDPuZ9OUB).

RT @ReadDark: If we can get the gravitational potential to fluctuate "significantly" on a timescale comparable to the local dynamical time,…

If we can get the gravitational potential to fluctuate "significantly" on a timescale comparable to the local dynamical time, then dark matter (DM) is "heated up": https://t.co/quC84uS2LA https://t.co/RrfrjrP3UP https://t.co/4uXRmn22VZ https://t.co/yYy…

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