ALMA Reveals Potential Evidence for Spiral Arms, Bars, and Rings in High-redshift Submillimeter Galaxies-Reference-Cited by-同舟云学术

ALMA Reveals Potential Evidence for Spiral Arms, Bars, and Rings in High-redshift Submillimeter Galaxies

Published:2019-05-13 Issue:2 Volume:876 Page:130
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Hodge J. A.^ORCID,Smail I.^ORCID,Walter F.^ORCID,Cunha E. da^ORCID,Swinbank A. M.^ORCID,Rybak M.^ORCID,Venemans B.^ORCID,Brandt W. N.^ORCID,Rivera G. Calistro,Chapman S. C.,Chen Chian-Chou^ORCID,Cox P.,Dannerbauer H.^ORCID,Decarli R.^ORCID,Greve T. R.^ORCID,Knudsen K. K.^ORCID,Menten K. M.^ORCID,Schinnerer E.^ORCID,Simpson J. M.^ORCID,Werf P. van der^ORCID,Wardlow J. L.,Weiss A.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab1846/pdf

Reference130 articles.

1. The X‐Ray Spectral Properties of SCUBA Galaxies

2. ASSESSING RADIATION PRESSURE AS A FEEDBACK MECHANISM IN STAR-FORMING GALAXIES

3. Morphology of bar orbits

4. What determines the strength and the slowdown rate of bars?

5. Bar formation and evolution in disc galaxies with gas and a triaxial halo: morphology, bar strength and halo properties

Cited by 105 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. Birds of a Feather: Resolving Stellar Mass Assembly with JWST/NIRCam in a Pair of Kindred z ∼ 2 Dusty Star-forming Galaxies Lensed by the PLCK G165.7+67.0 Cluster;The Astrophysical Journal;2024-09-01

2. JWST/CEERS sheds light on dusty star-forming galaxies: Forming bulges, lopsidedness, and outside-in quenching at cosmic noon;Astronomy & Astrophysics;2024-08

3. A 3D view on the local gravitational instability of cold gas discs in star-forming galaxies at 0 ≲ z ≲ 5;Astronomy & Astrophysics;2024-07

4. Turbulent Gas-rich Disks at High Redshift: Bars and Bulges in a Radial Shear Flow;The Astrophysical Journal;2024-06-01

5. Unveiling [C II] clumps in a lensed star-forming galaxy at z ∼ 3.4;Astronomy & Astrophysics;2024-05