ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13

Research output: Contribution to journal › Journal article › Research › peer-review

Standard

ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13. / Akins, Hollis B.; Fujimoto, Seiji; Finlator, Kristian; Watson, Darach; Knudsen, Kirsten K.; Richard, Johan; Bakx, Tom J. L. C.; Hashimoto, Takuya; Inoue, Akio K.; Matsuo, Hiroshi; Michalowski, Michal J.; Tamura, Yoichi.

In: Astrophysical Journal, Vol. 934, No. 1, 64, 02.07.2022.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Akins, HB, Fujimoto, S, Finlator, K, Watson, D, Knudsen, KK, Richard, J, Bakx, TJLC, Hashimoto, T, Inoue, AK, Matsuo, H, Michalowski, MJ & Tamura, Y 2022, 'ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13', Astrophysical Journal, vol. 934, no. 1, 64. https://doi.org/10.3847/1538-4357/ac795b

APA

Akins, H. B., Fujimoto, S., Finlator, K., Watson, D., Knudsen, K. K., Richard, J., Bakx, T. J. L. C., Hashimoto, T., Inoue, A. K., Matsuo, H., Michalowski, M. J., & Tamura, Y. (2022). ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13. Astrophysical Journal, 934(1), [64]. https://doi.org/10.3847/1538-4357/ac795b

Vancouver

Akins HB, Fujimoto S, Finlator K, Watson D, Knudsen KK, Richard J et al. ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13. Astrophysical Journal. 2022 Jul 2;934(1). 64. https://doi.org/10.3847/1538-4357/ac795b

Author

Akins, Hollis B. ; Fujimoto, Seiji ; Finlator, Kristian ; Watson, Darach ; Knudsen, Kirsten K. ; Richard, Johan ; Bakx, Tom J. L. C. ; Hashimoto, Takuya ; Inoue, Akio K. ; Matsuo, Hiroshi ; Michalowski, Michal J. ; Tamura, Yoichi. / ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13. In: Astrophysical Journal. 2022 ; Vol. 934, No. 1.

Bibtex

@article{a9c2f2ad1ecf49ddae734b7bb5f19c2e,

title = "ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13",

abstract = "We present spatially resolved morphological properties of [C II] 158 mu m, [O III] 88 mu m, dust, and rest-frame ultraviolet (UV) continuum emission for A1689-zD1, a strongly lensed, sub-L* galaxy at z = 7.13, by utilizing deep Atacama Large Millimeter/submillimeter Array (ALMA) and Hubble Space Telescope (HST) observations. While the [O III] line and UV continuum are compact, the [C II] line is extended up to a radius of r similar to 12 kpc. Using multi-band rest-frame far-infrared continuum data ranging from 52 to 400 mu m, we find an average dust temperature and emissivity index of Tdust=41-14+17 beta=1.7-0.7+1.1 6 galaxies.",

keywords = "PROBING COSMIC DAWN, HIGH-Z EXPLORATION, C II EMISSION, DUST CONTENT, INTERSTELLAR-MEDIUM, GALACTIC WINDS, MASS, REDSHIFT, LINE, QUASARS",

author = "Akins, {Hollis B.} and Seiji Fujimoto and Kristian Finlator and Darach Watson and Knudsen, {Kirsten K.} and Johan Richard and Bakx, {Tom J. L. C.} and Takuya Hashimoto and Inoue, {Akio K.} and Hiroshi Matsuo and Michalowski, {Michal J.} and Yoichi Tamura",

year = "2022",

month = jul,

day = "2",

doi = "10.3847/1538-4357/ac795b",

language = "English",

volume = "934",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "Institute of Physics Publishing, Inc",

number = "1",

}

RIS

TY - JOUR

T1 - ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13

AU - Akins, Hollis B.

AU - Fujimoto, Seiji

AU - Finlator, Kristian

AU - Watson, Darach

AU - Knudsen, Kirsten K.

AU - Richard, Johan

AU - Bakx, Tom J. L. C.

AU - Hashimoto, Takuya

AU - Inoue, Akio K.

AU - Matsuo, Hiroshi

AU - Michalowski, Michal J.

AU - Tamura, Yoichi

PY - 2022/7/2

Y1 - 2022/7/2

N2 - We present spatially resolved morphological properties of [C II] 158 mu m, [O III] 88 mu m, dust, and rest-frame ultraviolet (UV) continuum emission for A1689-zD1, a strongly lensed, sub-L* galaxy at z = 7.13, by utilizing deep Atacama Large Millimeter/submillimeter Array (ALMA) and Hubble Space Telescope (HST) observations. While the [O III] line and UV continuum are compact, the [C II] line is extended up to a radius of r similar to 12 kpc. Using multi-band rest-frame far-infrared continuum data ranging from 52 to 400 mu m, we find an average dust temperature and emissivity index of Tdust=41-14+17 beta=1.7-0.7+1.1 6 galaxies.

AB - We present spatially resolved morphological properties of [C II] 158 mu m, [O III] 88 mu m, dust, and rest-frame ultraviolet (UV) continuum emission for A1689-zD1, a strongly lensed, sub-L* galaxy at z = 7.13, by utilizing deep Atacama Large Millimeter/submillimeter Array (ALMA) and Hubble Space Telescope (HST) observations. While the [O III] line and UV continuum are compact, the [C II] line is extended up to a radius of r similar to 12 kpc. Using multi-band rest-frame far-infrared continuum data ranging from 52 to 400 mu m, we find an average dust temperature and emissivity index of Tdust=41-14+17 beta=1.7-0.7+1.1 6 galaxies.

KW - PROBING COSMIC DAWN

KW - HIGH-Z EXPLORATION

KW - C II EMISSION

KW - DUST CONTENT

KW - INTERSTELLAR-MEDIUM

KW - GALACTIC WINDS

KW - MASS

KW - REDSHIFT

KW - LINE

KW - QUASARS

U2 - 10.3847/1538-4357/ac795b

DO - 10.3847/1538-4357/ac795b

M3 - Journal article

VL - 934

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 64

ER -

ID: 316057115