GOALS-JWST: NIRCam and MIRI Imaging of the Circumnuclear Starburst Ring in NGC 7469

被引:7
|
作者
Bohn, Thomas [1 ]
Inami, Hanae [1 ]
Diaz-Santos, Tanio [2 ,3 ]
Armus, Lee [4 ]
Linden, S. T. [5 ]
Vivian, U. [6 ]
Surace, Jason [4 ]
Larson, Kirsten L. [7 ]
Evans, Aaron S. [8 ,9 ]
Hoshioka, Shunshi [1 ]
Lai, Thomas [4 ]
Song, Yiqing [8 ,9 ]
Mazzarella, Joseph M. [4 ]
Barcos-Munoz, Loreto [8 ,9 ]
Charmandaris, Vassilis [2 ,3 ,10 ]
Howell, Justin H. [4 ]
Medling, Anne M. [11 ,12 ,13 ]
Privon, George C. [8 ,14 ]
Rich, Jeffrey A. [15 ]
Stierwalt, Sabrina [16 ]
Aalto, Susanne [17 ]
Boker, Torsten [18 ]
Brown, Michael J. I. [19 ]
Iwasawa, Kazushi [20 ,21 ]
Malkan, Matthew A. [22 ]
van der Werf, Paul P. [23 ]
Appleton, Philip [4 ]
Hayward, Christopher C. [24 ]
Kemper, Francisca [21 ,25 ,26 ]
Law, David [27 ]
Marshall, Jason [28 ]
Murphy, Eric J. [8 ]
Sanders, David [29 ]
机构
[1] Hiroshima Univ, Hiroshima Astrophys Sci Ctr, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, Japan
[2] Fdn Res & Technol Hellas FORTH, Inst Astrophys, Iraklion 70013, Greece
[3] European Univ Cyprus, Sch Sci, Diogenes St, CY-1516 Nicosia, Cyprus
[4] CALTECH, IPAC, 1200 E Calif Blvd, Pasadena, CA 91125 USA
[5] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
[6] Univ Calif Irvine, Dept Phys & Astron, 4129 Frederick Reines Hall, Irvine, CA 92697 USA
[7] AURA European Space Agcy ESA, Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[8] Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA
[9] Univ Virginia, Dept Astron, 530 McCormick Rd, Charlottesville, VA 22903 USA
[10] Univ Crete, Dept Phys, Iraklion 71003, Greece
[11] Univ Toledo, Dept Phys & Astron, Toledo, OH 43606 USA
[12] Univ Toledo, Ritter Astrophys Res Ctr, Toledo, OH 43606 USA
[13] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Canberra, ACT, Australia
[14] Univ Florida, Dept Astron, POB 112055, Gainesville, FL 32611 USA
[15] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA
[16] Occidental Coll, Phys Dept, 1600 Campus Rd, Los Angeles, CA 90042 USA
[17] Chalmers Univ Technol, Dept Space Earth & Environm, SE-41296 Gothenburg, Sweden
[18] European Space Agcy, Space Telescope Sci Inst, Baltimore, MD 21218 USA
[19] Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
[20] Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, Marti i Franques 1, E-08028 Barcelona, Spain
[21] ICREA, Pg Lluis Co 23, E-08010 Barcelona, Spain
[22] UCLA, Dept Phys & Astron, Los Angeles, CA 90095 USA
[23] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands
[24] Flatiron Inst, Ctr Computat Astrophys, 162 Fifth Ave, New York, NY 10010 USA
[25] CSIC, ICE, Can Magrans S-N, E-08193 Barcelona, Spain
[26] Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain
[27] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[28] Glendale Community Coll, 1500 N Verdugo Rd, Glendale, CA 91208 USA
[29] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
基金
欧洲研究理事会; 瑞典研究理事会; 美国国家科学基金会;
关键词
LUMINOUS INFRARED GALAXIES; WEBB-SPACE-TELESCOPE; RESOLUTION MIDINFRARED OBSERVATIONS; ACTIVE GALACTIC NUCLEI; YOUNG STAR-CLUSTERS; ALMA OBSERVATIONS; LINE REGION; OUTFLOWS; MASS; GAS;
D O I
10.3847/2041-8213/acab61
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present James Webb Space Telescope (JWST) imaging of NGC 7469 with the Near-Infrared Camera and the Mid-InfraRed Instrument. NGC 7469 is a nearby, z = 0.01627, luminous infrared galaxy that hosts both a Seyfert Type-1.5 nucleus and a circumnuclear starburst ring with a radius of & SIM;0.5 kpc. The new near-infrared (NIR) JWST imaging reveals 66 star-forming regions, 37 of which were not detected by Hubble Space Telescope (HST) observations. Twenty-eight of the 37 sources have very red NIR colors that indicate obscurations up to A (v) & SIM; 7 and a contribution of at least 25% from hot dust emission to the 4.4 & mu;m band. Their NIR colors are also consistent with young (<5 Myr) stellar populations and more than half of them are coincident with the mid-infrared (MIR) emission peaks. These younger, dusty star-forming regions account for & SIM;6% and & SIM;17% of the total 1.5 and 4.4 & mu;m luminosity of the starburst ring, respectively. Thanks to JWST, we find a significant number of young dusty sources that were previously unseen due to dust extinction. The newly identified 28 young sources are a significant increase compared to the number of HST-detected young sources (4-5). This makes the total percentage of the young population rise from & SIM;15% to 48%. These results illustrate the effectiveness of JWST in identifying and characterizing previously hidden star formation in the densest star-forming environments around active galactic nuclei (AGN).
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页数:8
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