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Title: Nebular spectra of 111 Type Ia supernovae disfavour single-degenerate progenitors

Abstract

ABSTRACT We place statistical constraints on Type Ia supernova (SN Ia) progenitors using 227 nebular-phase spectra of 111 SNe Ia. We find no evidence of stripped companion emission in any of the nebular-phase spectra. Upper limits are placed on the amount of mass that could go undetected in each spectrum using recent hydrodynamic simulations. With these null detections, we place an observational 3σ upper limit on the fraction of SNe Ia that are produced through the classical H-rich non-degenerate companion scenario of $$\lt 5.5 {{\ \rm per\ cent}}$$. Additionally, we set a tentative 3σ upper limit otan He star progenitor scenarios of $$\lt 6.4 {{\ \rm per\ cent}}$$, although further theoretical modelling is required. These limits refer to our most representative sample including normal, 91bg-like, 91T-like, and ‘super-Chandrasekhar’ SNe Ia but excluding SNe Iax and SNe Ia-CSM. As part of our analysis, we also derive a Nebular Phase Phillips Relation, which approximates the brightness of an SN Ia from 150 to 500 d after maximum using the peak magnitude and decline rate parameter Δm15(B).

Authors:
ORCiD logo [1];  [1]; ORCiD logo [2];  [3];  [4];  [5];  [3];  [6];  [2];  [7]; ORCiD logo [8];  [9];  [9];  [10];  [11];  [11];  [12];  [3]
+ Show Author Affiliations
  1. Institute for Astronomy, University of Hawai‘i at Manoa, 2680 Woodlawn Dr., Honolulu, Hi 96822, USA
  2. Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA
  3. Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA, Center for Cosmology and AstroParticle Physics (CCAPP), The Ohio State University, 191 W. Woodruff Avenue, Columbus, OH 43210, USA
  4. Núcleo de Astronomía de la Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile, Millennium Institute of Astrophysics, Santiago, Chile
  5. Physics Department, University of California, Berkeley, CA 94720, USA
  6. European Southern Observatory, Alonso de Cordova 3107 Casilla 19001, Vitacura, Santiago, Chile
  7. PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA
  8. Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, USA
  9. Department of Physics, Florida State University, 77 Chieftan Way, Tallahassee, FL 32306, USA
  10. Finnish Centre for Astronomy with ESO (FINCA), University of Turku, FI-20014 Turku, Finland, Tuorla Observatory, Department of Physics and Astronomy, University of Turku, FI-20014 Turku, Finland
  11. Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena, Chile
  12. Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
Publication Date:
Research Org.:
Krell Institute, Ames, IA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1601006
Alternate Identifier(s):
OSTI ID: 1803687
Grant/Contract Number:  
SC0019323
Resource Type:
Published Article
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 493 Journal Issue: 1; Journal ID: ISSN 0035-8711
Publisher:
Oxford University Press
Country of Publication:
United Kingdom
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; supernovae, general; galaxies, distances and redshifts

Citation Formats

Tucker, M. A., Shappee, B. J., Vallely, P. J., Stanek, K. Z., Prieto, J. L., Botyanszki, J., Kochanek, C. S., Anderson, J. P., Brown, J., Galbany, L., Holoien, T. W-S, Hsiao, E. Y., Kumar, S., Kuncarayakti, H., Morrell, N., Phillips, M. M., Stritzinger, M. D., and Thompson, Todd A. Nebular spectra of 111 Type Ia supernovae disfavour single-degenerate progenitors. United Kingdom: N. p., 2019. Web. doi:10.1093/mnras/stz3390.
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Tucker, M. A., Shappee, B. J., Vallely, P. J., Stanek, K. Z., Prieto, J. L., Botyanszki, J., Kochanek, C. S., Anderson, J. P., Brown, J., Galbany, L., Holoien, T. W-S, Hsiao, E. Y., Kumar, S., Kuncarayakti, H., Morrell, N., Phillips, M. M., Stritzinger, M. D., & Thompson, Todd A. Nebular spectra of 111 Type Ia supernovae disfavour single-degenerate progenitors. United Kingdom. https://doi.org/10.1093/mnras/stz3390
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Tucker, M. A., Shappee, B. J., Vallely, P. J., Stanek, K. Z., Prieto, J. L., Botyanszki, J., Kochanek, C. S., Anderson, J. P., Brown, J., Galbany, L., Holoien, T. W-S, Hsiao, E. Y., Kumar, S., Kuncarayakti, H., Morrell, N., Phillips, M. M., Stritzinger, M. D., and Thompson, Todd A. Wed . "Nebular spectra of 111 Type Ia supernovae disfavour single-degenerate progenitors". United Kingdom. https://doi.org/10.1093/mnras/stz3390.
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@article{osti_1601006,
title = {Nebular spectra of 111 Type Ia supernovae disfavour single-degenerate progenitors},
author = {Tucker, M. A. and Shappee, B. J. and Vallely, P. J. and Stanek, K. Z. and Prieto, J. L. and Botyanszki, J. and Kochanek, C. S. and Anderson, J. P. and Brown, J. and Galbany, L. and Holoien, T. W-S and Hsiao, E. Y. and Kumar, S. and Kuncarayakti, H. and Morrell, N. and Phillips, M. M. and Stritzinger, M. D. and Thompson, Todd A.},
abstractNote = {ABSTRACT We place statistical constraints on Type Ia supernova (SN Ia) progenitors using 227 nebular-phase spectra of 111 SNe Ia. We find no evidence of stripped companion emission in any of the nebular-phase spectra. Upper limits are placed on the amount of mass that could go undetected in each spectrum using recent hydrodynamic simulations. With these null detections, we place an observational 3σ upper limit on the fraction of SNe Ia that are produced through the classical H-rich non-degenerate companion scenario of $\lt 5.5 {{\ \rm per\ cent}}$. Additionally, we set a tentative 3σ upper limit otan He star progenitor scenarios of $\lt 6.4 {{\ \rm per\ cent}}$, although further theoretical modelling is required. These limits refer to our most representative sample including normal, 91bg-like, 91T-like, and ‘super-Chandrasekhar’ SNe Ia but excluding SNe Iax and SNe Ia-CSM. As part of our analysis, we also derive a Nebular Phase Phillips Relation, which approximates the brightness of an SN Ia from 150 to 500 d after maximum using the peak magnitude and decline rate parameter Δm15(B).},
doi = {10.1093/mnras/stz3390},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 493,
place = {United Kingdom},
year = {2019},
month = {12}
}
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The Evolution of Early‐Type Galaxies in Distant Clusters. II. Internal Kinematics of 55 Galaxies in the \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=0.33$ \end{document} Cluster Cl 1358+62
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Gaia Data Release 2 : Summary of the contents and survey properties
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ESI, a New Keck Observatory Echellette Spectrograph and Imager
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Kinematics of the Local Universe: XIII. 21-cm line measurements of 452 galaxies with the Nançay radiotelescope,
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NORMAL TYPE Ia SUPERNOVAE FROM VIOLENT MERGERS OF WHITE DWARF BINARIES
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THE CARNEGIE SUPERNOVA PROJECT: INTRINSIC COLORS OF TYPE Ia SUPERNOVAE
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A significantly off-centre 56Ni distribution for the low-luminosity type Ia supernova SN 2016brx from the 100IAS survey★
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The Carnegie Supernova Project: The Low‐Redshift Survey
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ON THE PROGENITOR SYSTEM OF THE TYPE Iax SUPERNOVA 2014dt IN M61
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CONSTRAINING THE SPIN-DOWN TIMESCALE OF THE WHITE DWARF PROGENITORS OF TYPE Ia SUPERNOVAE
journal, November 2013

Berkeley Supernova Ia Program - I. Observations, data reduction and spectroscopic sample of 582 low-redshift Type Ia supernovae: BSNIP I: SN Ia spectra
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Balmer-dominated Shocks Exclude Hot Progenitors for Many Type Ia Supernovae
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The DEIMOS spectrograph for the Keck II Telescope: integration and testing
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THE CARNEGIE SUPERNOVA PROJECT: ANALYSIS OF THE FIRST SAMPLE OF LOW-REDSHIFT TYPE-Ia SUPERNOVAE
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Detection of a Light Echo from SN 1998[CLC]bu[/CLC]
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[ITAL]BVRI[/ITAL] Light Curves for 22 Type I[CLC]a[/CLC] Supernovae
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Nebular Spectroscopy of Kepler ’s Brightest Supernova
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THE IMPACT OF TYPE Ia SUPERNOVA EXPLOSIONS ON HELIUM COMPANIONS IN THE CHANDRASEKHAR-MASS EXPLOSION SCENARIO
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THE Pan-STARRS1 PHOTOMETRIC SYSTEM
journal, April 2012

EEV large-format CCD camera on the WHT ISIS spectrograph
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Sub-Chandrasekhar mass models for Type IA supernovae
journal, March 1994

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THE SPECTROSCOPIC DIVERSITY OF TYPE Ia SUPERNOVAE
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CONSTRAINING TYPE Ia SUPERNOVAE PROGENITORS FROM THREE YEARS OF SUPERNOVA LEGACY SURVEY DATA
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No Stripped Companion Material in the Nebular Spectrum of the “Two-Component” Type Ia Supernova ASASSN-18bt
journal, February 2019

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Late stages of the evolution of close compact binaries: Type I supernovae, gamma-ray bursts, and supersoft X-ray sources
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Comprehensive observations of the bright and energetic Type Iax SN 2012Z: Interpretation as a Chandrasekhar mass white dwarf explosion
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An Open Catalog for Supernova Data
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K2 Observations of SN 2018oh Reveal a Two-component Rising Light Curve for a Type Ia Supernova
journal, December 2018

Gaia Data Release 2 : Photometric content and validation
journal, August 2018

Automated data reduction workflows for astronomy: The ESO Reflex environment
journal, November 2013

Three-dimensional simulations of the interaction between Type Ia supernova ejecta and their main sequence companions
journal, November 2012

RESULTS OF THE LICK OBSERVATORY SUPERNOVA SEARCH FOLLOW-UP PHOTOMETRY PROGRAM: BVRI LIGHT CURVES OF 165 TYPE Ia SUPERNOVAE
journal, September 2010

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IMACS: The Inamori-Magellan Areal Camera and Spectrograph on Magellan-Baade
journal, March 2011

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Nebular H α Limits for Fast Declining SNe Ia
journal, May 2019

TYPE Iax SUPERNOVAE: A NEW CLASS OF STELLAR EXPLOSION
journal, March 2013

Optical Observations of the Supernova in NGC 5253
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Photometry of Supernova 1972 IN NGC 5253
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Non‐LTE Model Atmosphere Analysis of the Large Magellanic Cloud Supersoft X‐Ray Source CAL 83
journal, January 2005

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OPTICAL SPECTROSCOPY OF TYPE Ia SUPERNOVAE
journal, March 2008

Accreting white dwarf models for type I supernovae. I - Presupernova evolution and triggering mechanisms
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Detection of Circumstellar Material in a Normal Type Ia Supernova
journal, August 2007

Type I supernovae. I - Analytic solutions for the early part of the light curve
journal, February 1982

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Seeing Double: ASASSN-18bt Exhibits a Two-component Rise in the Early-time K2 Light Curve
journal, December 2018

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Greatly enhanced eccentricity oscillations in quadruple systems composed of two binaries: implications for stars, planets and transients
journal, August 2013

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  • Monthly Notices of the Royal Astronomical Society, Vol. 435, Issue 2
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Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations
journal, December 2018

SINGLE-DEGENERATE TYPE Ia SUPERNOVAE WITHOUT HYDROGEN CONTAMINATION
journal, March 2011

Physical dust Models for the Extinction Toward Supernova 2014j in m82
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UBVRI Light Curves of 44 Type Ia Supernovae
journal, January 2006

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A deep Search for Prompt Radio Emission from Thermonuclear Supernovae with the very Large Array
journal, April 2016

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Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?
journal, May 2010

PREDICTING THE AMOUNT OF HYDROGEN STRIPPED BY THE SN EXPLOSION FOR SN 2002cx-LIKE SNe Ia
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On the Hydrogen Emission from the Type Ia Supernova SN 2002ic
journal, March 2004

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The Diversity of Type Ia Supernovae: Evidence for Systematics?
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The Gaia mission
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Observational properties of thermonuclear supernovae
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An upper limit on the contribution of accreting white dwarfs to the type Ia supernova rate
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WISeREP—An Interactive Supernova Data Repository
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The Faint Object Spectrograph for the 2.5-m Isaac Newton Telescope
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The Extinction Properties of and Distance to the Highly Reddened Type IA Supernova 2012cu
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Nebular spectra and abundance tomography of the Type Ia supernova SN 2011fe: a normal SN Ia with a stable Fe core
journal, May 2015

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ASASSN-15pz: Revealing Significant Photometric Diversity among 2009dc-like, Peculiar SNe Ia
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Double-degenerate semidetached binaries with helium secondaries: cataclysmic variables, supersoft X-ray sources, supernovae and accretion-induced collapses
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SN 2002cx: The Most Peculiar Known Type Ia Supernova
journal, April 2003

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Have the Elusive Progenitors of Type Ia Supernovae Been Discovered?
journal, August 2003

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Merging of binary white dwarfs, neutron stars and black holes under the influence of gravitational wave radiation
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Rapid eccentricity oscillations and the mergers of compact objects in hierarchical triples
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How Do Type Ia Supernova Nebular Spectra Depend on Explosion Properties? Insights from Systematic Non-LTE Modeling
journal, August 2017

The first binary star evolution model producing a Chandrasekhar mass white dwarf
journal, November 2003

The ejected mass distribution of Type Ia supernovae: a significant rate of non-Chandrasekhar-mass progenitors
journal, October 2014

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Explosions of Sub--Chandrasekhar Mass White Dwarfs in Two Dimensions
journal, October 1995

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THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE
journal, October 2011

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  • The Astronomical Journal, Vol. 142, Issue 5
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Imprints of the ejecta–companion interaction in Type Ia supernovae: main-sequence, subgiant, and red giant companions
journal, October 2016

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  • Monthly Notices of the Royal Astronomical Society, Vol. 465, Issue 2
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Cepheid Distances to SNe Ia Host Galaxies Based on a Revised Photometric Zero Point of the HST WFPC2 and New PL Relations and Metallicity Corrections
journal, July 2006

  • Saha, A.; Thim, F.; Tammann, G. A.
  • The Astrophysical Journal Supplement Series, Vol. 165, Issue 1
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Extensive HST ultraviolet spectra and multiwavelength observations of SN 2014J in M82 indicate reddening and circumstellar scattering by typical dust
journal, August 2014

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  • Monthly Notices of the Royal Astronomical Society, Vol. 443, Issue 4
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Where are the double-degenerate progenitors of Type Ia supernovae?
journal, November 2018

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  • Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 3
  • DOI: 10.1093/mnras/sty2965

The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances
journal, January 2001

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  • DOI: 10.1086/318301

THE PECULIAR EXTINCTION LAW OF SN 2014J MEASURED WITH THE HUBBLE SPACE TELESCOPE
journal, May 2014

Identification of the Companion Stars of Type Ia supernovae
journal, March 2001

  • Canal, R.; Méndez, J.; Ruiz-Lapuente, P.
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  • DOI: 10.1086/319479

Carnegie Supernova Project-II: Extending the Near-infrared Hubble Diagram for Type Ia Supernovae to z ∼ 0.1
journal, November 2018

  • Phillips, M. M.; Contreras, Carlos; Hsiao, E. Y.
  • Publications of the Astronomical Society of the Pacific, Vol. 131, Issue 995
  • DOI: 10.1088/1538-3873/aae8bd

TYPE Ia SINGLE DEGENERATE SURVIVORS MUST BE OVERLUMINOUS
journal, February 2013

The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star
journal, September 2006

  • Andrew Howell, D.; Sullivan, Mark; Nugent, Peter E.
  • Nature, Vol. 443, Issue 7109
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The Wide Field Spectrograph (WiFeS)
journal, May 2007

  • Dopita, Michael; Hart, John; McGregor, Peter
  • Astrophysics and Space Science, Vol. 310, Issue 3-4
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NO STRIPPED HYDROGEN IN THE NEBULAR SPECTRA OF NEARBY TYPE Ia SUPERNOVA 2011fe
journal, December 2012

COSMICFLOWS-2 : THE DATA
journal, September 2013

  • Tully, R. Brent; Courtois, Hélène M.; Dolphin, Andrew E.
  • The Astronomical Journal, Vol. 146, Issue 4
  • DOI: 10.1088/0004-6256/146/4/86
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