Discovery of Multiple Ultra-broad-velocity Molecular Features Associated with the W44 Molecular Cloud

Abstract We report the discovery of multiple compact molecular features exhibiting extremely broad velocity widths toward the W44 molecular cloud. Atacama Large Millimeter/submillimeter Array CO J = 3–2 data reveal eight “Petit-Bullets” surrounding the previously known “Bullet.” Each Petit-Bullet shows a distinct V-shaped structure in position–velocity space, reminiscent of the Y-shaped morphology of the Bullet, suggesting a common origin. These features are interpreted as the result of high-velocity plunges of compact gravitational objects into dense molecular gas. The spatial and kinematic properties of the Petit-Bullets suggest that the plunging material was not a single object but rather a small cluster of compact bodies. A virial mass of 1.0 × 10 5 M ⊙ inferred from their velocity dispersion is comparable to that of typical globular clusters. Momentum analysis further implies that the main Bullet likely formed by an isolated black hole. These findings provide new evidence for dynamical interactions between halo clusters and disk molecular gas.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2026-02-23
DOI
https://doi.org/10.3847/2041-8213/ae36aa
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
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article

Discovery of Multiple Ultra-broad-velocity Molecular Features Associated with the W44 Molecular Cloud

Shiho Tsujimoto, T. Kotani, Momoko Makita, Tomoharu Oka
The Astrophysical Journal Letters
Astrophysics and Star Formation Studies
article

Discovery of Multiple Ultra-broad-velocity Molecular Features Associated with the W44 Molecular Cloud

Shiho Tsujimoto, T. Kotani, Momoko Makita, Tomoharu Oka
article en

Abstract

Abstract We report the discovery of multiple compact molecular features exhibiting extremely broad velocity widths toward the W44 molecular cloud. Atacama Large Millimeter/submillimeter Array CO J = 3–2 data reveal eight “Petit-Bullets” surrounding the previously known “Bullet.” Each Petit-Bullet shows a distinct V-shaped structure in position–velocity space, reminiscent of the Y-shaped morphology of the Bullet, suggesting a common origin. These features are interpreted as the result of high-velocity plunges of compact gravitational objects into dense molecular gas. The spatial and kinematic properties of the Petit-Bullets suggest that the plunging material was not a single object but rather a small cluster of compact bodies. A virial mass of 1.0 × 10 5 M ⊙ inferred from their velocity dispersion is comparable to that of typical globular clusters. Momentum analysis further implies that the main Bullet likely formed by an isolated black hole. These findings provide new evidence for dynamical interactions between halo clusters and disk molecular gas.

The Astrophysical Journal LettersVol. 999(1)
Keio University (JP)
Openalex Percentile: Top 46%
Astrophysics and Star Formation Studies
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Discovery of Multiple Ultra-broad-velocity Molecular Features Associated with the W44 Molecular Cloud — Shiho Tsujimoto, T. Kotani, et al. · The Astrophysical Journal Letters (2026) | TGRS Research Map | TGRS