The Type II-plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor
We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN) 2017eaw in NGC 6946. SN 2017eaw is a normal SN II-P intermediate in properties between, for example, SN 1999em and SN 2012aw and the more luminous...
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Published in | The Astrophysical journal Vol. 875; no. 2; pp. 136 - 158 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
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Philadelphia
The American Astronomical Society
20.04.2019
IOP Publishing |
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Abstract | We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN) 2017eaw in NGC 6946. SN 2017eaw is a normal SN II-P intermediate in properties between, for example, SN 1999em and SN 2012aw and the more luminous SN 2004et, also in NGC 6946. We have determined that the extinction to SN 2017eaw is primarily due to the Galactic foreground and that the SN site metallicity is likely subsolar. We have also independently confirmed a tip-of-the-red-giant-branch (TRGB) distance to NGC 6946 of 7.73 0.78 Mpc. The distances to the SN that we have also estimated via both the standardized candle method and expanding photosphere method corroborate the TRGB distance. We confirm the SN progenitor identity in pre-explosion archival Hubble Space Telescope (HST) and Spitzer Space Telescope images, via imaging of the SN through our HST Target of Opportunity program. Detailed modeling of the progenitor's spectral energy distribution indicates that the star was a dusty, luminous red supergiant consistent with an initial mass of ∼15 M . |
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AbstractList | We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN) 2017eaw in NGC 6946. SN 2017eaw is a normal SN II-P intermediate in properties between, for example, SN 1999em and SN 2012aw and the more luminous SN 2004et, also in NGC 6946. We have determined that the extinction to SN 2017eaw is primarily due to the Galactic foreground and that the SN site metallicity is likely subsolar. We have also independently confirmed a tip-of-the-red-giant-branch (TRGB) distance to NGC 6946 of 7.73 ± 0.78 Mpc. The distances to the SN that we have also estimated via both the standardized candle method and expanding photosphere method corroborate the TRGB distance. We confirm the SN progenitor identity in pre-explosion archival
Hubble Space Telescope
(
HST
) and
Spitzer Space Telescope
images, via imaging of the SN through our
HST
Target of Opportunity program. Detailed modeling of the progenitor’s spectral energy distribution indicates that the star was a dusty, luminous red supergiant consistent with an initial mass of ∼15
M
⊙
. We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN) 2017eaw in NGC 6946. SN 2017eaw is a normal SN II-P intermediate in properties between, for example, SN 1999em and SN 2012aw and the more luminous SN 2004et, also in NGC 6946. We have determined that the extinction to SN 2017eaw is primarily due to the Galactic foreground and that the SN site metallicity is likely subsolar. We have also independently confirmed a tip-of-the-red-giant-branch (TRGB) distance to NGC 6946 of 7.73 ± 0.78 Mpc. The distances to the SN that we have also estimated via both the standardized candle method and expanding photosphere method corroborate the TRGB distance. We confirm the SN progenitor identity in pre-explosion archival Hubble Space Telescope (HST) and Spitzer Space Telescope images, via imaging of the SN through our HST Target of Opportunity program. Detailed modeling of the progenitor’s spectral energy distribution indicates that the star was a dusty, luminous red supergiant consistent with an initial mass of ∼15 M ⊙. We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN) 2017eaw in NGC 6946. SN 2017eaw is a normal SN II-P intermediate in properties between, for example, SN 1999em and SN 2012aw and the more luminous SN 2004et, also in NGC 6946. We have determined that the extinction to SN 2017eaw is primarily due to the Galactic foreground and that the SN site metallicity is likely subsolar. We have also independently confirmed a tip-of-the-red-giant-branch (TRGB) distance to NGC 6946 of 7.73 0.78 Mpc. The distances to the SN that we have also estimated via both the standardized candle method and expanding photosphere method corroborate the TRGB distance. We confirm the SN progenitor identity in pre-explosion archival Hubble Space Telescope (HST) and Spitzer Space Telescope images, via imaging of the SN through our HST Target of Opportunity program. Detailed modeling of the progenitor's spectral energy distribution indicates that the star was a dusty, luminous red supergiant consistent with an initial mass of ∼15 M . |
Author | Piro, Anthony L. Hestenes, Julia C. Wilson, Richard Kumar, Sahana Maund, Justyn R. Yunus, Sameen Fox, Ori D. Kelly, Patrick L. Howard, Andrew W. Channa, Sanyum Morozova, Viktoriya Crossfield, Ian J. M. Stegman, Samantha M. de Jaeger, Thomas Zheng, WeiKang Ross, Timothy W. Isaacson, Howard Milisavljevic, Dan Kosiarek, Molly R. Leonard, Douglas C. Conner, Brody Smith, Nathan Littlefair, Stuart P. Butterley, Timothy Brink, Thomas G. Andrews, Jennifer E. Dhillon, Vik S. Jeffers, Benjamin T. Zhang, Keto Van Dyk, Schuyler D. Long, Knox S. Filippenko, Alexei V. Srinivasan, Sundar Falcon, Edward |
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Cherry Avenue, Tucson, AZ 85721, USA – sequence: 7 givenname: Nathan surname: Smith fullname: Smith, Nathan organization: University of Arizona Steward Observatory, 933 N. Cherry Avenue, Tucson, AZ 85721, USA – sequence: 8 givenname: Douglas C. surname: Leonard fullname: Leonard, Douglas C. organization: San Diego State University Department of Astronomy, San Diego, CA 92182-1221, USA – sequence: 9 givenname: Viktoriya orcidid: 0000-0002-0674-5930 surname: Morozova fullname: Morozova, Viktoriya organization: Princeton University Department of Astrophysical Sciences, Princeton, NJ 08544, USA – sequence: 10 givenname: Alexei V. orcidid: 0000-0003-3460-0103 surname: Filippenko fullname: Filippenko, Alexei V. organization: University of California Miller Senior Fellow, Miller Institute for Basic Research in Science, Berkeley, CA 94720, USA – sequence: 11 givenname: Brody surname: Conner fullname: Conner, Brody organization: Purdue University Department of Physics and Astronomy, 525 Northwestern Avenue, West Lafayette, IN 47907, USA – sequence: 12 givenname: Dan orcidid: 0000-0002-0763-3885 surname: Milisavljevic fullname: Milisavljevic, Dan organization: Purdue University Department of Physics and Astronomy, 525 Northwestern Avenue, West Lafayette, IN 47907, USA – sequence: 13 givenname: Thomas surname: de Jaeger fullname: de Jaeger, Thomas organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 14 givenname: Knox S. orcidid: 0000-0002-4134-864X surname: Long fullname: Long, Knox S. organization: Eureka Scientific, Inc. 2452 Delmer Street, Suite 100, Oakland, CA 94602-3017, USA – sequence: 15 givenname: Howard orcidid: 0000-0002-0531-1073 surname: Isaacson fullname: Isaacson, Howard organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 16 givenname: Ian J. M. surname: Crossfield fullname: Crossfield, Ian J. M. organization: Massachusetts Institute of Technology Department of Physics, 77 Massachusetts Avenue, Cambridge, MA, USA – sequence: 17 givenname: Molly R. orcidid: 0000-0002-6115-4359 surname: Kosiarek fullname: Kosiarek, Molly R. organization: University of California Santa Cruz , Santa Cruz, CA 95064, USA – sequence: 18 givenname: Andrew W. orcidid: 0000-0001-8638-0320 surname: Howard fullname: Howard, Andrew W. organization: California Institute of Technology , Pasadena, CA 91125, USA – sequence: 19 givenname: Ori D. orcidid: 0000-0003-2238-1572 surname: Fox fullname: Fox, Ori D. organization: Space Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA – sequence: 20 givenname: Patrick L. orcidid: 0000-0003-3142-997X surname: Kelly fullname: Kelly, Patrick L. organization: University of Minnesota College of Science & Engineering, Minnesota Institute for Astrophysics, 115 Union St. SE, Minneapolis, MN 55455, USA – sequence: 21 givenname: Anthony L. orcidid: 0000-0001-6806-0673 surname: Piro fullname: Piro, Anthony L. organization: The Observatories of the Carnegie Institution for Science , 813 Santa Barbara Street, Pasadena, CA 91101, USA – sequence: 22 givenname: Stuart P. orcidid: 0000-0001-7221-855X surname: Littlefair fullname: Littlefair, Stuart P. organization: University of Sheffield Department of Physics and Astronomy, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK – sequence: 23 givenname: Vik S. surname: Dhillon fullname: Dhillon, Vik S. organization: Instituto de Astrofísica de Canarias , E-38205 La Laguna, Tenerife, Spain – sequence: 24 givenname: Richard surname: Wilson fullname: Wilson, Richard organization: University of Durham Center for Advanced Instrumentation, Department of Physics, South Road, Durham DH1 3LE, UK – sequence: 25 givenname: Timothy surname: Butterley fullname: Butterley, Timothy organization: University of Durham Center for Advanced Instrumentation, Department of Physics, South Road, Durham DH1 3LE, UK – sequence: 26 givenname: Sameen surname: Yunus fullname: Yunus, Sameen organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 27 givenname: Sanyum surname: Channa fullname: Channa, Sanyum organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 28 givenname: Benjamin T. surname: Jeffers fullname: Jeffers, Benjamin T. organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 29 givenname: Edward surname: Falcon fullname: Falcon, Edward organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 30 givenname: Timothy W. surname: Ross fullname: Ross, Timothy W. organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 31 givenname: Julia C. surname: Hestenes fullname: Hestenes, Julia C. organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 32 givenname: Samantha M. surname: Stegman fullname: Stegman, Samantha M. organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 33 givenname: Keto surname: Zhang fullname: Zhang, Keto organization: University of California Department of Astronomy, Berkeley, CA 94720-3411, USA – sequence: 34 givenname: Sahana surname: Kumar fullname: Kumar, Sahana organization: Florida State University Department of Physics, 77 Chieftain Way, Tallahassee, FL 32306, USA |
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Copyright | 2019. The American Astronomical Society. All rights reserved. Copyright IOP Publishing Apr 20, 2019 |
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Snippet | We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN)... |
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SubjectTerms | Astrophysics galaxies: distances and redshifts galaxies: individual (NGC 6946) Hubble Space Telescope Metallicity Photosphere Red giant stars Space telescopes Spectral energy distribution stars: massive Supergiant stars supergiants Supernova supernovae: general supernovae: individual (SN 2017eaw) |
Title | The Type II-plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor |
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