One-kiloparsec expanding cylinder of H i gas around the Galactic Center

Author:

Sofue Yoshiaki1

Affiliation:

1. Institute of Astronomy, The University of Tokyo , 2-21-1 Osawa Mitaka, Tokyo 181-0015, Japan

Abstract

Abstract We report the discovery of an expanding cylinder of H i gas of radius 1 kpc and vertical extent 800 pc by analyzing the 21 cm line survey data from the literature. The cylinder is expanding at 150 km s−1, rotating at 100 km s−1, and is interpreted as due to a high-velocity conical wind from the Galactic Center. The total mass of the cylinder is estimated to be ∼8.5 × 105M⊙ and kinetic energy ∼3 × 1053 erg.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. On the Hα faintness of the North Polar Spur;Monthly Notices of the Royal Astronomical Society;2023-07-03

2. A galactic breeze origin for the Fermi bubbles emission;Monthly Notices of the Royal Astronomical Society;2022-12-01

3. Living on the edge of the Milky Way's central molecular zone;Astronomy & Astrophysics;2022-12

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