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arxiv.org arXiv
arxiv.org › abs › astro-ph › 0510198v1
Many of the known extrasolar planets are ``hot Jupiters,'' giant planets with orbital periods of just a few days. We use the observed distribution of hot Jupiters to constrain the location of the ``in...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0610102v2
There is currently debate over whether the dust content of planetary systems is stochastically regenerated or originates in planetesimal belts evolving in steady state. In this paper a simple model fo...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 9710142v1
A definite prediction from recent N-body/hydro simulations of the structure formation of the universe is the presence of a diffuse intergalactic medium (IGM) in a temperature range of 10^5 - 10^7 K. T...
arxiv.org arXiv
arxiv.org › abs › 0907.1795v1
What is long-baseline optical/IR stellar interferometry? A few years ago, many astronomers might not have been able to answer that question properly. This is today hopefully not the case anymore, beca...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0511336v1
Recent Spitzer infrared (IR) observations of two transiting hot Jupiters during their secondary eclipses have provided the first direct detection of planets orbiting other stars (Charbonneau et al. 20...
arxiv.org arXiv
arxiv.org › abs › 0812.3792v2
We study the nature of the covariant thermodynamic geometry arising from the free energy of hot QCD. We systematically analyze the underlying equilibrium thermodynamic configurations of the free energ...
arxiv.org arXiv
arxiv.org › abs › 1112.2140v1
Since its discovery as an X-ray source with the Einstein Observatory, the hot X-ray emitting interstellar medium of early-type galaxies has been studied intensively, with observations of improving qua...
arxiv.org arXiv
arxiv.org › abs › 1308.2447v2
We started a new project which aims to find compact hot subdwarf binaries at low Galactic latitudes. Targets are selected from several photometric surveys and a spectroscopic follow-up campaign to fin...
arxiv.org arXiv
arxiv.org › abs › 1510.04173v1
Thanks to the high sensitivity of the instruments on board the XMM-Newton and Chandra satellites, it has become possible to explore the properties of the X-ray emission from hot subdwarfs. The small b...
arxiv.org arXiv
arxiv.org › abs › 2002.08257v1
The hot circum-galactic medium (CGM) represents the hot gas distributed beyond the stellar content of the galaxies while typically within their dark matter halos. It serves as a depository of energy a...