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Yakov Faerman

Researcher at Tel Aviv University

Publications -  14
Citations -  357

Yakov Faerman is an academic researcher from Tel Aviv University. The author has contributed to research in topics: Milky Way & Galaxy. The author has an hindex of 7, co-authored 10 publications receiving 277 citations. Previous affiliations of Yakov Faerman include The Racah Institute of Physics.

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Massive warm/hot galaxy coronae as probed by uv/x-ray oxygen absorption and emission. i. basic model

TL;DR: In this paper, an analytic phenomenological model for extended warm/hot gaseous coronae of galaxies is presented, where the authors consider UV OVI COS-Halos absorption line data in combination with Milky Way X-ray OVII and OVIII absorption and emission.
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Massive warm/hot galaxy coronae - II. Isentropic model

TL;DR: In this paper, a new analytic phenomenological model for the extended circumgalactic material (CGM) of galaxies is presented, where the warm/hot gas is in hydrostatic equilibrium in a MW gravitational potential and a pressure component with an adiabatic index of 4/3 is included to approximate the effects of a magnetic field and cosmic rays.
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Ultra-compact High Velocity Clouds as Minihalos and Dwarf Galaxies

TL;DR: In this article, dark matter minihalo models for the Ultra-Compact, High-Velocity H I Clouds (UCHVCs) recently discovered in the 21?cm ALFALFA survey were presented.
Journal ArticleDOI

Massive Warm/Hot Galaxy Coronae as Probed by UV/X-ray Oxygen Absorption and Emission: I - Basic Model

TL;DR: In this paper, an analytic phenomenological model for extended warm/hot gaseous coronae of galaxies is presented, where the authors consider UV OVI COS-Halos absorption line data in combination with Milky Way X-ray OVII and OVIII absorption and emission.
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AGC198606 : A gas-bearing dark matter minihalo?

TL;DR: In this paper, neutral hydrogen (H i) imaging observations with the Westerbork Synthesis Radio Telescope of AGC198606, an H i cloud discovered in the ALFALFA 21cm survey, reveal a smooth undisturbed H i morphology with a full extent of 23' × 16' at the 5 × 1018 atoms cm-2 level.