Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6905
Title: Extraplanar X-ray emission from disc-wide out ows in spiral galaxies.
Authors: Vijayan, Aditi
Sarkar, Kartick Chandra
Nath, Biman B.
Sharma, Prateek
Shchekinov, Yuri
Keywords: Galaxies Starburst
X-rays
Issue Date: Apr-2018
Publisher: Oxford University Press for the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2018, Vol. 475, p5513-5528
Abstract: We study the effects of mass and energy injection due to OB associations spread across the rotating disc of a Milky Way-type galaxy, with the help of three-dimensional (3D) hydrodynamic simulations. We compare the resulting X-ray emission with that produced from the injection of mass and energy from a central region. We find that the predicted X-ray image shows a filamentary structure that arises even in the absence of disc gas inhomogeneity. This structure stems from warm clumps made of disc material being lifted by the injected gas. We show that as much as half of the total X-ray emission comes from regions surrounding warm clumps that are made of a mix of disc and injected gas. This scenario has the potential to explain the origin of the observed extraplanar X-ray emission around star-forming galaxies and can be used to understand the observed sub-linear relation between the LX, the total X-ray luminosity, and star formation rate (SFR). We quantify the mass contained in these ‘bow-shock’ regions. We also show that the top-most region of the outer shock above the central area emits harder X-rays than the rest. Further, we find that the mass distribution in different temperature ranges is bimodal, peaking at 104–105 K (in warm clumps) and 106–107 K (X-ray emitting gas). The mass-loading factor is found to decrease with increasing SFR, consistent with previous theoretical estimates and simulations.
Description: Open Access
URI: http://hdl.handle.net/2289/6905
ISSN: 0035-8711
1365-2966 (Online)
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1712.06252
https://arxiv.org/abs/1712.06252
http://dx.doi.org/10.1093/mnras/sty198
Copyright: 2018 The authors & the Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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