A gravitationally unstable gas disk of a starburst galaxy 12 billion years ago
Ken-ichi Tadaki, Daisuke Iono, Min S. Yun, Itziar Aretxaga, Bunyo, Hatsukade, David H. Hughes, So Ikarashi, Takuma Izumi, Ryohei Kawabe, Kotaro, Kohno, Minju Lee, Yuichi Matsuda, Kohichiro Nakanishi, Toshiki Saito, Yoichi, Tamura, Junko Ueda, Hideki Umehata, Grant W. Wilson

TL;DR
This study provides high-resolution observations of a distant starburst galaxy, revealing a gravitationally unstable gas disk that drives intense star formation in the early Universe.
Contribution
First detailed spatial and kinematic mapping of molecular gas in a high-redshift starburst galaxy's core, showing gravitational instability as a key star formation mechanism.
Findings
Gas disk is clumpy and rotation-supported.
The gas is gravitationally unstable.
Star formation timescale is about 100 million years.
Abstract
Submillimeter bright galaxies in the early Universe are vigorously forming stars at ~1000 times higher rate than the Milky Way. A large fraction of stars is formed in the central 1 kiloparsec region, that is comparable in size to massive, quiescent galaxies found at the peak of the cosmic star formation history, and eventually the core of giant elliptical galaxies in the present-day Universe. However, the physical and kinematic properties inside a compact starburst core are poorly understood because dissecting it requires angular resolution even higher than the Hubble Space Telescope can offer. Here we report 550 parsec-resolution observations of gas and dust in the brightest unlensed submillimeter galaxy at z=4.3. We map out for the first time the spatial and kinematic structure of molecular gas inside the heavily dust-obscured core. The gas distribution is clumpy while the underlying…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
