「火山の氷」が銀河中心のガス雲年齢を解明(‘Ice in a Volcano’ Reveals Age of Gas Cloud at Milky Way’s Center)

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2025-07-07 ノースカロライナ州立大学 (NCState)

ノースカロライナ州立大学の研究チームは、ミルキーウェイ中心のフェルミバブル内に冷たい中性水素雲を発見した。これは超高温ガスに包まれた「火山の中の氷」のような構造で、数百万年の寿命を持つ比較的若い現象と判明。観測はグリーンバンク電波望遠鏡を用いて行われた。フェルミバブルの年齢も従来の1,000万年以上から数百万年へ見直され、銀河のエネルギー循環や進化モデルに新たな視点を提供する発見となった。

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北フェルミバブルに巻き込まれた新しい高緯度Hi雲複合体 A New High-latitude H i Cloud Complex Entrained in the Northern Fermi Bubble

Rongmon Bordoloi, Andrew J. Fox, and Felix J. Lockman
The Astrophysical Journal Letters  Published: 2025 July 7
DOI:10.3847/2041-8213/addd16

「火山の氷」が銀河中心のガス雲年齢を解明(‘Ice in a Volcano’ Reveals Age of Gas Cloud at Milky Way’s Center)

Abstract

We report the discovery of 11 high-velocity H i clouds at Galactic latitudes of 25°–30°, likely embedded in the Milky Way’s nuclear wind. The clouds are detected with deep Green Bank Telescope 21 cm observations of a 3:2 × 6:2 field around QSO 1H1613-097, located behind the northern Fermi Bubble. Our measurements reach 3σ limits on NHI as low as 3.1 × 1017 cm−2, more than twice as sensitive as previous H i studies of the bubbles. The clouds span −180 ≤ vLSR ≤ −90 km s−1 and are the highest-latitude 21 cm high-velocity cloud detected inside the bubbles. Eight clouds are spatially resolved, showing coherent structures with sizes of 4–28 pc, peak column densities of log(NHI/cm2) = 17.9–18.7, and H i masses up to 1470 M. Several exhibit internal velocity gradients. Their presence at such high latitudes is surprising, given the short expected survival times for clouds expelled from the Galactic center. These objects may be fragments of a larger cloud disrupted by interaction with the surrounding hot gas.

1701物理及び化学
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