PHANGS-JWST First Results: The Dust Filament Network of NGC 628 and Its Relation to Star Formation Activity

被引:23
|
作者
Thilker, David A. [1 ]
Lee, Janice C. [2 ]
Deger, Sinan [3 ,4 ]
Barnes, Ashley T. [5 ]
Bigiel, Frank [5 ]
Boquien, Mederic [6 ]
Cao, Yixian [7 ]
Chevance, Melanie [8 ,9 ]
Dale, Daniel A. [10 ]
Egorov, Oleg V. [8 ,11 ]
Glover, Simon C. O. [12 ]
Grasha, Kathryn [13 ]
Henshaw, Jonathan D. [14 ,15 ]
Klessen, Ralf S. [12 ,16 ]
Koch, Eric [17 ]
Kruijssen, J. M. Diederik [9 ]
Leroy, Adam K. [18 ]
Lessing, Ryan A. [1 ]
Meidt, Sharon E. [19 ]
Pinna, Francesca [15 ]
Querejeta, Miguel [20 ]
Rosolowsky, Erik [21 ]
Sandstrom, Karin M. [22 ]
Schinnerer, Eva
Smith, Rowan J. [23 ]
Watkins, Elizabeth J. [8 ]
Williams, Thomas G. [15 ]
Anand, Gagandeep S. [24 ]
Belfiore, Francesco [25 ]
Blanc, Guillermo A. [26 ,27 ]
Chandar, Rupali [28 ]
Congiu, Enrico [27 ]
Emsellem, Eric [29 ,30 ]
Groves, Brent [13 ,31 ]
Kreckel, Kathryn [8 ]
Larson, Kirsten L. [32 ]
Liu, Daizhong [33 ]
Pessa, Ismael [15 ,34 ]
Whitmore, Bradley C. [24 ]
机构
[1] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[2] NSF's NOIRLab, Gemini Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA
[3] CALTECH, 1200 E Calif Blvd,MC 249-17, Pasadena, CA 91125 USA
[4] Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, SE-10691 Stockholm, Sweden
[5] Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany
[6] Univ Antofagasta, Ctr Astron CITEVA, Ave Angamos 601, Antofagasta, Chile
[7] Max Planck Inst Extraterr Phys MPE, Giessenbachstr 1, D-85748 Garching, Germany
[8] Heidelberg Univ, Astron Rechen Inst, Zent Astron, Monchhofstr 12-14, D-69120 Heidelberg, Germany
[9] Cosm Origins Life COOL Res DAO, Salt Lake City, UT USA
[10] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA
[11] Lomonosov Moscow State Univ, Sternberg Astron Inst, Univ Sky Pr 13, Moscow 119234, Russia
[12] Heidelberg Univ, Inst Theoret Astrophys, Zent Astron, Albert Ueberle Str 2, D-69120 Heidelberg, Germany
[13] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia
[14] Liverpool John Moores Univ, Astrophys Res Inst, 146 Brownlow Hill, Liverpool L3 5RF, England
[15] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
[16] Heidelberg Univ, Interdisziplinares Zent Wissensch Rechnen, Neuenheimer Feld 205, D-69120 Heidelberg, Germany
[17] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[18] Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA
[19] Univ Ghent, Sterrenkundig Observ, Krijgslaan 281 S9, B-9000 Ghent, Belgium
[20] Observ Astron Nacl IGN, C Alfonso XII,3, E-28014 Madrid, Spain
[21] Univ Alberta, Dept Phys, Edmonton, AB T6G 2E1, Canada
[22] Univ Calif San Diego, Ctr Astrophys & Space Sci, Dept Phys, 9500 Gilman Dr, La Jolla, CA 92093 USA
[23] Univ Manchester, Jodrell Bank Ctr Astrophys, Dept Phys & Astron, Oxford Rd, Manchester M13 9PL, England
[24] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[25] INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50157 Florence, Italy
[26] Observ Carnegie Inst Sci, 813 St Barbara St, Pasadena, CA 91101 USA
[27] Univ Chile, Dept Astron, Camino Observ 1515, Santiago, Chile
[28] Univ Toledo, 2801 W Bancroft St,Mail Stop 111, Toledo, OH 43606 USA
[29] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
[30] Univ Lyon 1, Univ Lyon, Ctr Rech Astrophys Lyon UMR5574, ENS Lyon,CNRS, F-69230 St Genis Laval, France
[31] Univ Western Australia, Int Ctr Radio Astron Res, 35 Stirling Highway, Crawley, WA 6009, Australia
[32] Space Telescope Sci Inst, AURA European Space Agcy ESA, 3700 San Martin Dr, Baltimore, MD 21218 USA
[33] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany
[34] Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany
基金
欧洲研究理事会; 加拿大自然科学与工程研究理事会; 澳大利亚研究理事会;
关键词
MOLECULAR FILAMENTS; INTERSTELLAR-MEDIUM; FORMING FILAMENTS; NEARBY GALAXIES; EMISSION; MILKY; CLOUDS; SCALE; GAS; IDENTIFICATION;
D O I
10.3847/2041-8213/acaeac
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
PHANGS-JWST mid-infrared (MIR) imaging of nearby spiral galaxies has revealed ubiquitous filaments of dust emission in intricate detail. We present a pilot study to systematically map the dust filament network (DFN) at multiple scales between 25 and 400 pc in NGC 628. MIRI images at 7.7, 10, 11.3, and 21 mu m of NGC 628 are used to generate maps of the filaments in emission, while PHANGS-HST B-band imaging yields maps of dust attenuation features. We quantify the correspondence between filaments traced by MIR thermal continuum/polycyclic aromatic hydrocarbon (PAH) emission and filaments detected via extinction/scattering of visible light; the fraction of MIR flux contained in the DFN; and the fraction of H ii regions, young star clusters, and associations within the DFN. We examine the dependence of these quantities on the physical scale at which the DFN is extracted. With our highest-resolution DFN maps (25 pc filament width), we find that filaments in emission and attenuation are cospatial in 40% of sight lines, often exhibiting detailed morphological agreement; that similar to 30% of the MIR flux is associated with the DFN; and that 75%-80% of the star formation in H ii regions and 60% of the mass in star clusters younger than 5 Myr are contained within the DFN. However, the DFN at this scale is anticorrelated with looser associations of stars younger than 5 Myr identified using PHANGS-HST near-UV imaging. We discuss the impact of these findings on studies of star formation and the interstellar medium, and the broad range of new investigations enabled by multiscale maps of the DFN.
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页数:19
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