Distances to PHANGS galaxies: New tip of the red giant branch measurements and adopted distances

被引：143

作者：

Anand, Gagandeep S. ^{[1
,2
]}

Lee, Janice C. ^{[1
]}

Van Dyk, Schuyler D. ^{[1
]}

Leroy, Adam K. ^{[3
]}

Rosolowsky, Erik ^{[4
]}

Schinnerer, Eva ^{[5
]}

Larson, Kirsten ^{[1
]}

Kourkchi, Ehsan ^{[2
]}

Kreckel, Kathryn ^{[6
]}

Scheuermann, Fabian ^{[6
]}

Rizzi, Luca ^{[7
]}

Thilker, David ^{[8
]}

Tully, R. Brent ^{[2
]}

Bigiel, Frank ^{[9
]}

Blanc, Guillermo A. ^{[10
,11
]}

Boquien, Mederic ^{[12
]}

Chandar, Rupali ^{[13
]}

Dale, Daniel ^{[14
]}

Emsellem, Eric ^{[15
,16
]}

Deger, Sinan ^{[1
]}

Glover, Simon C. O. ^{[17
]}

Grasha, Kathryn ^{[18
]}

Groves, Brent ^{[18
,19
]}

Klessen, Ralf S. ^{[17
,20
]}

Kruijssen, J. M. Diederik ^{[21
]}

Querejeta, Miguel ^{[22
]}

Sanchez-Blazquez, Patricia ^{[23
]}

Schruba, Andreas ^{[24
]}

Turner, Jordan ^{[14
]}

Ubeda, Leonardo ^{[25
]}

Williams, Thomas G. ^{[5
]}

Whitmore, Brad ^{[25
]}

机构：

[1] CALTECH, IPAC, Pasadena, CA 91125 USA

[2] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

[3] Ohio State Univ, Dept Astron, 4055 McPherson Lab,140 West 18th Ave, Columbus, OH 43210 USA

[4] Univ Alberta, Dept Phys, 4-183 CCIS, Edmonton, AB T6G 2E1, Canada

[5] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[6] Zentrum Astron Univ Heidelberg, Astron Rechen Inst, Monchhofstr 12-14, D-69120 Heidelberg, Germany

[7] WM Keck Observ, 65-1120 Mamalahoa Highway, Kamuela, HI 96743 USA

[8] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

[9] Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany

[10] Observ Carnegie Inst Sci, Pasadena, CA 91101 USA

[11] Univ Chile, Dept Astron, Santiago, Chile

[12] Univ Antofagasta, Ctr Astron CITEVA, Ave Angamos 601, Antofagasta 1270300, Chile

[13] Univ Toledo, Dept Phys & Astron, Toledo, OH 43606 USA

[14] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA

[15] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[16] Univ Lyon, ENS Lyon, Ctr Rech Astrophys Lyon UMR5574, CNRS, F-69230 St Genis Laval, France

[17] Heidelberg Univ, Zentrum Astron, Inst Theoret Astrophys, Albert Ueberle Str 2, D-69120 Heidelberg, Germany

[18] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia

[19] Univ Western Australia, Int Ctr Radio Astron Res, 35 Stirling Hwy, Crawley, WA 6009, Australia

[20] Heidelberg Univ, Interdisziplinares Zentrum Wissensch Rechnen, Neuenheimer Feld 205, D-69120 Heidelberg, Germany

[21] Heidelberg Univ, Astron Rechen Inst, Zentrum Astron, Monchhofstr 12-14, D-69120 Heidelberg, Germany

[22] Observ Astron Nacl IGN, C Alfonso 12 3, E-28014 Madrid, Spain

[23] Univ Complutense Madrid, Fac CC Fis, E-28040 Madrid, Spain

[24] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany

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

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2021年 / 501卷 / 03期

基金：

加拿大自然科学与工程研究理事会; 欧洲研究理事会; 美国国家科学基金会; 美国国家航空航天局;

关键词：

galaxies: fundamental parameters; galaxies: stellar content; distance scale; HUBBLE CONSTANT; DWARF GALAXIES; PECULIAR VELOCITIES; ROBUST TIP; CALIBRATION; INDICATOR; CLUSTER; MOTION; CLOUD; DISK;

D O I：

10.1093/mnras/staa3668

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

PHANGS-HST is an ultraviolet-optical imaging survey of 38 spiral galaxies within similar to 20 Mpc. Combined with the PHANGS-ALMA, PHANGS-MUSE surveys and other multiwavelength data, the data set will provide an unprecedented look into the connections between young stars, HII regions, and cold molecular gas in these nearby star-forming galaxies. Accurate distances are needed to transform measured observables into physical parameters (e.g. brightness to luminosity, angular to physical sizes of molecular clouds, star clusters and associations). PHANGS-HST has obtained parallel ACS imaging of the galaxy haloes in the F606W and F814W bands. Where possible, we use these parallel fields to derive tip of the red giant branch (TRGB) distances to these galaxies. In this paper, we present TRGB distances for 10 PHANGS galaxies from similar to 4 to similar to 15 Mpc, based on the first year of PHANGS-HST observations. Four of these represent the first published TRGB distance measurements (IC 5332, NGC 2835, NGC 4298, and NGC 4321), and seven of which are the best available distances to these targets. We also provide a compilation of distances for the 118 galaxies in the full PHANGS sample, which have been adopted for the first PHANGS-ALMA public data release.

引用

页码：3621 / 3639

页数：19

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