First Look at z > 1 Bars in the Rest-frame Near-infrared with JWST Early CEERS Imaging

被引：58

作者：

Guo, Yuchen ^{[1
]}

Jogee, Shardha ^{[1
]}

Finkelstein, Steven L. ^{[1
]}

Chen, Zilei ^{[1
]}

Wise, Eden ^{[1
]}

Bagley, Micaela B. ^{[1
]}

Barro, Guillermo ^{[2
]}

Wuyts, Stijn ^{[3
]}

Kocevski, Dale D. ^{[4
]}

Kartaltepe, Jeyhan S. ^{[5
]}

McGrath, Elizabeth J. ^{[4
]}

Ferguson, Henry C. ^{[6
]}

Mobasher, Bahram ^{[7
]}

Giavalisco, Mauro ^{[8
]}

Lucas, Ray A. ^{[6
]}

Zavala, Jorge A. ^{[9
]}

Lotz, Jennifer M. ^{[10
]}

Grogin, Norman A. ^{[6
]}

Huertas-Company, Marc ^{[11
,12
,13
]}

Vega-Ferrero, Jesus ^{[11
]}

Hathi, Nimish P. ^{[6
]}

Haro, Pablo Arrabal ^{[14
]}

Dickinson, Mark ^{[14
]}

Koekemoer, Anton M. ^{[6
]}

Papovich, Casey ^{[15
,16
]}

Pirzkal, Nor ^{[17
]}

Aaron Yung, L. Y. ^{[18
]}

Backhaus, Bren E. ^{[19
]}

Bell, Eric F. ^{[20
]}

Calabro, Antonello ^{[21
]}

Cleri, Nikko J. ^{[15
,16
]}

Coogan, Rosemary T. ^{[22
]}

Cooper, M. C. ^{[23
]}

Costantin, Luca ^{[24
]}

Croton, Darren ^{[25
,26
]}

Davis, Kelcey ^{[27
]}

Dekel, Avishai ^{[28
]}

Franco, Maximilien ^{[1
]}

Gardner, Jonathan P. ^{[18
]}

Holwerda, Benne W. ^{[29
]}

Hutchison, Taylor A. ^{[18
]}

Pandya, Viraj ^{[30
]}

Perez-Gonzalez, Pablo G. ^{[31
]}

Ravindranath, Swara ^{[6
]}

Rose, Caitlin ^{[5
]}

Trump, Jonathan R. ^{[19
]}

de la Vega, Alexander ^{[32
]}

Wang, Weichen ^{[33
]}

机构：

[1] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA

[2] Univ Pacific, Dept Phys, Stockton, CA 90340 USA

[3] Univ Bath, Dept Phys, Bath BA2 7AY, England

[4] Colby Coll, Dept Phys & Astron, Waterville, ME 04901 USA

[5] Rochester Inst Technol, Sch Phys & Astron, Lab Multiwavelength Astrophys, 84 Lomb Mem Dr, Rochester, NY 14623 USA

[6] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[7] Univ Calif Riverside, Dept Phys & Astron, 900 Univ Ave, Riverside, CA 92521 USA

[8] Univ Massachusetts Amherst, 710 North Pleasant St, Amherst, MA 01003 USA

[9] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[10] NSFs Natl Opt Infrared Astron Res Lab, Gemini Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA

[11] Inst Astrofis Canarias, Tenerife, Spain

[12] Univ La Laguna, Tenerife, Spain

[13] Univ Paris Cite, LERMA Observ Paris, PSL, Paris, France

[14] NSFs Natl Opt Infrared Astron Res Lab, 950 N Cherry Ave, Tucson, AZ 85719 USA

[15] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA

[16] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA

[17] ESA AURA Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[18] NASA Goddard Space Flight Ctr, Astrophys Sci Div, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[19] Univ Connecticut, Dept Phys, 196A Auditorium Rd,Unit 3046, Storrs, CT 06269 USA

[20] Univ Michigan, Dept Astron, 1085 S Univ Ave, Ann Arbor, MI 48109 USA

[21] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Rome, Italy

[22] Univ Paris Cite, Univ Paris Saclay, Sorbonne Paris Cite, CEA,IRFU,DAp,AIM,CNRS, F-91191 Gif Sur Yvette, France

[23] Univ Calif Irvine, Dept Phys & Astron, 4129 Reines Hall, Irvine, CA 92697 USA

[24] Ctr Astrobiol CSIC INTA, Ctra Ajalvir Km 4, E-28850 Madrid, Spain

[25] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

[26] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Canberra, ACT, Australia

[27] Univ Connecticut, Dept Phys, 196 Auditorium Rd,Unit 3046, Storrs, CT 06269 USA

[28] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel

[29] Univ Louisville, Phys & Astron Dept, Louisville, KY 40292 USA

[30] Columbia Univ, Columbia Astrophys Lab, 550 West 120th St, New York, NY 10027 USA

[31] CSIC INTA, Ctr Astrobiol CAB, Ctra Ajalvir Km 4, E-28850 Madrid, Spain

[32] Univ Calif Riverside, Dept Phys & Astron, Riverside, CA 92521 USA

[33] Johns Hopkins Univ, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2023年 / 945卷 / 01期

关键词：

COSMOLOGY LEGACY SURVEY; BARRED SPIRAL GALAXIES; 8 BILLION YEARS; EGS DEEP FIELD; SECULAR EVOLUTION; STAR-FORMATION; DISC GALAXIES; STRUCTURAL-PROPERTIES; ELLIPTIC GALAXIES; CENTRAL REGION;

D O I：

10.3847/2041-8213/acacfb

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Stellar bars are key drivers of secular evolution in galaxies and can be effectively studied using rest-frame near-infrared (NIR) images, which trace the underlying stellar mass and are less impacted by dust and star formation than rest-frame UV or optical images. We leverage the power of JWST CEERS NIRCam images to present the first quantitative identification and characterization of stellar bars at z > 1 based on rest-frame NIR F444W images of high resolution (similar to 1.3 kpc at z similar to 1-3). We identify stellar bars in these images using quantitative criteria based on ellipse fits. For this pilot study, we present six examples of robustly identified bars at z > 1 with spectroscopic redshifts, including the two highest-redshift bars at z similar to 2.136 and 2.312 quantitatively identified and characterized to date. The stellar bars at z similar to 1.1-2.3 presented in our study have projected semimajor axes of similar to 2.9-4.3 kpc and projected ellipticities of similar to 0.41-0.53 in the rest-frame NIR. The barred host galaxies have stellar masses similar to 1 x 10(10) to 2 x 10(11) M (circle dot) and star formation rates of similar to 21-295 M (circle dot) yr(-1), and several have potential nearby companions. Our finding of bars at z similar to 1.1-2.3 demonstrates the early onset of such instabilities and supports simulations where bars form early in massive dynamically cold disks. It also suggests that if these bars at lookback times of 8-11 Gyr survive out to present epochs, bar-driven secular processes may operate over a long time and have a significant impact on some galaxies by z similar to 0.

引用

页数：13

共 33 条

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