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On the consequences of the gravothermal catastrophe

Donald Lynden-Bell, +1 more
- 01 Jul 1980 - 
- Vol. 191, Iss: 3, pp 483-498
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1980-07-01 and is currently open access. It has received 215 citations till now. The article focuses on the topics: Gravitational collapse.

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Young Massive Star Clusters

TL;DR: A review of the current state of the art in observations and dynamical modeling of young massive star clusters can be found in this paper, where the authors focus on star clusters younger than 100$ Myr, more than a few current crossing times old, and more massive than 10^4$Msun.
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Statistical mechanics of gravitating systems

TL;DR: The statistical description of a system containing a large number of particles which interact via Newtonian gravity is discussed in this paper, which exhibits several peculiarities due to the long range, unshielded nature of the gravitational interaction.
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Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA

TL;DR: In this paper, a review of the current state of knowledge and an outline of some of the outstanding questions that still need to be addressed is provided, based on discussions at a workshop hosted by the Albert Einstein Institute in Golm, Germany.
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Negative specific heat in astronomy, physics and chemistry

TL;DR: In this article, the authors review progress in the understanding of gravitational thermodynamics and pinpoint the error in the proof that all systems have positive specific heat and say when it can occur and discuss the development of the thermal runaway in both the gravothermal catastrophe and its inverse.
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Phase transitions in self-gravitating systems

TL;DR: In this paper, the authors compare the microcanonical evolution of stellar systems from the canonical evolution of self-gravitating Brownian particles, and show that at low energies, self-aggravitating Hamiltonian systems experience a gravothermal catastrophe in the micro-canonical ensemble.