Type II supernovae in low-luminosity host galaxies

Physics

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https://doi.org/10.1093/mnras/sty1581
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Galaxies: general, Supernovae: general

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Type II supernovae in low-luminosity host galaxies. / Gutiérrez, C. P.; Anderson, J P ; Sullivan, M. et al.
In: Monthly Notices of the Royal Astronomical Society, Vol. 479, No. 3, 21.09.2018, p. 3232-3253.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Gutiérrez, CP, Anderson, JP, Sullivan, M, Dessart, L, González-Gaitan, S, Galbany, L, Dimitriadis, G, Arcavi, I, Bufano, F, Chen, T-W, Dennefeld, M, Gromadzki, M, Haislip, JB, Hosseinzadeh, G, Howell, DA, Inserra, C, Kankare, E, Leloudas, G, Maguire, K, McCully, C, Morrell, N, Olivares, EF, Pignata, G, Reichart, DE, Reynolds, T, Smartt, SJ, Sollerman, J, Taddia, F, Takáts, K, Terreran, G, Valenti, S & Young, DR 2018, 'Type II supernovae in low-luminosity host galaxies', Monthly Notices of the Royal Astronomical Society, vol. 479, no. 3, pp. 3232-3253. https://doi.org/10.1093/mnras/sty1581

APA

Gutiérrez, C. P., Anderson, J. P., Sullivan, M., Dessart, L., González-Gaitan, S., Galbany, L., Dimitriadis, G., Arcavi, I., Bufano, F., Chen, T.-W., Dennefeld, M., Gromadzki, M., Haislip, J. B., Hosseinzadeh, G., Howell, D. A., Inserra, C., Kankare, E., Leloudas, G., Maguire, K., ... Young, D. R. (2018). Type II supernovae in low-luminosity host galaxies. Monthly Notices of the Royal Astronomical Society, 479(3), 3232-3253. https://doi.org/10.1093/mnras/sty1581

Vancouver

Gutiérrez CP, Anderson JP, Sullivan M, Dessart L, González-Gaitan S, Galbany L et al. Type II supernovae in low-luminosity host galaxies. Monthly Notices of the Royal Astronomical Society. 2018 Sept 21;479(3):3232-3253. Epub 2018 Jun 15. doi: 10.1093/mnras/sty1581

Author

Gutiérrez, C. P. ; Anderson, J P ; Sullivan, M. et al. / Type II supernovae in low-luminosity host galaxies. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 479, No. 3. pp. 3232-3253.

Bibtex

@article{605a1f97218c45128041cb05b83610a8,

title = "Type II supernovae in low-luminosity host galaxies",

abstract = "We present an analysis of a new sample of type II core-collapse supernovae (SNe II) occurring within low-luminosity galaxies, comparing these with a sample of events in brighter hosts. Our analysis is performed comparing SN II spectral and photometric parameters and estimating the influence of metallicity (inferred from host luminosity differences) on SN II transient properties. We measure the SN absolute magnitude at maximum, the light-curve plateau duration, the optically thick duration, and the plateau decline rate in the V band, together with expansion velocities and pseudo-equivalent-widths (pEWs) of several absorption lines in the SN spectra. For the SN host galaxies, we estimate the absolute magnitude and the stellar mass, a proxy for the metallicity of the host galaxy. SNe II exploding in low-luminosity galaxies display weaker pEWs of Fe II λ5018, confirming the theoretical prediction that metal lines in SN II spectra should correlate with metallicity.We also find that SNe II in low-luminosity hosts have generally slower declining light curves and display weaker absorption lines. We find no relationship between the plateau duration or the expansion velocities with SN environment, suggesting that the hydrogen envelope mass and the explosion energy are not correlated with the metallicity of the host galaxy. This result supports recent predictions that mass-loss for red supergiants is independent of metallicity.",

keywords = "Galaxies: general, Supernovae: general",

author = "Guti{\'e}rrez, {C. P.} and Anderson, {J P} and M. Sullivan and L. Dessart and S. Gonz{\'a}lez-Gaitan and L. Galbany and G. Dimitriadis and I. Arcavi and F. Bufano and T-W Chen and M. Dennefeld and M. Gromadzki and Haislip, {J. B.} and G. Hosseinzadeh and Howell, {D. A.} and C. Inserra and E. Kankare and G. Leloudas and K. Maguire and C. McCully and N. Morrell and Olivares, {E. F.} and G. Pignata and Reichart, {D. E.} and T. Reynolds and Smartt, {S. J.} and J. Sollerman and F. Taddia and K. Tak{\'a}ts and G. Terreran and S. Valenti and Young, {D. R.}",

note = "Publisher Copyright: {\textcopyright} 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.",

year = "2018",

month = sep,

day = "21",

doi = "10.1093/mnras/sty1581",

language = "English",

volume = "479",

pages = "3232--3253",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "OXFORD UNIV PRESS",

number = "3",

}

RIS

TY - JOUR

T1 - Type II supernovae in low-luminosity host galaxies

AU - Gutiérrez, C. P.

AU - Anderson, J P

AU - Sullivan, M.

AU - Dessart, L.

AU - González-Gaitan, S.

AU - Galbany, L.

AU - Dimitriadis, G.

AU - Arcavi, I.

AU - Bufano, F.

AU - Chen, T-W

AU - Dennefeld, M.

AU - Gromadzki, M.

AU - Haislip, J. B.

AU - Hosseinzadeh, G.

AU - Howell, D. A.

AU - Inserra, C.

AU - Kankare, E.

AU - Leloudas, G.

AU - Maguire, K.

AU - McCully, C.

AU - Morrell, N.

AU - Olivares, E. F.

AU - Pignata, G.

AU - Reichart, D. E.

AU - Reynolds, T.

AU - Smartt, S. J.

AU - Sollerman, J.

AU - Taddia, F.

AU - Takáts, K.

AU - Terreran, G.

AU - Valenti, S.

AU - Young, D. R.

PY - 2018/9/21

Y1 - 2018/9/21

N2 - We present an analysis of a new sample of type II core-collapse supernovae (SNe II) occurring within low-luminosity galaxies, comparing these with a sample of events in brighter hosts. Our analysis is performed comparing SN II spectral and photometric parameters and estimating the influence of metallicity (inferred from host luminosity differences) on SN II transient properties. We measure the SN absolute magnitude at maximum, the light-curve plateau duration, the optically thick duration, and the plateau decline rate in the V band, together with expansion velocities and pseudo-equivalent-widths (pEWs) of several absorption lines in the SN spectra. For the SN host galaxies, we estimate the absolute magnitude and the stellar mass, a proxy for the metallicity of the host galaxy. SNe II exploding in low-luminosity galaxies display weaker pEWs of Fe II λ5018, confirming the theoretical prediction that metal lines in SN II spectra should correlate with metallicity.We also find that SNe II in low-luminosity hosts have generally slower declining light curves and display weaker absorption lines. We find no relationship between the plateau duration or the expansion velocities with SN environment, suggesting that the hydrogen envelope mass and the explosion energy are not correlated with the metallicity of the host galaxy. This result supports recent predictions that mass-loss for red supergiants is independent of metallicity.

AB - We present an analysis of a new sample of type II core-collapse supernovae (SNe II) occurring within low-luminosity galaxies, comparing these with a sample of events in brighter hosts. Our analysis is performed comparing SN II spectral and photometric parameters and estimating the influence of metallicity (inferred from host luminosity differences) on SN II transient properties. We measure the SN absolute magnitude at maximum, the light-curve plateau duration, the optically thick duration, and the plateau decline rate in the V band, together with expansion velocities and pseudo-equivalent-widths (pEWs) of several absorption lines in the SN spectra. For the SN host galaxies, we estimate the absolute magnitude and the stellar mass, a proxy for the metallicity of the host galaxy. SNe II exploding in low-luminosity galaxies display weaker pEWs of Fe II λ5018, confirming the theoretical prediction that metal lines in SN II spectra should correlate with metallicity.We also find that SNe II in low-luminosity hosts have generally slower declining light curves and display weaker absorption lines. We find no relationship between the plateau duration or the expansion velocities with SN environment, suggesting that the hydrogen envelope mass and the explosion energy are not correlated with the metallicity of the host galaxy. This result supports recent predictions that mass-loss for red supergiants is independent of metallicity.

KW - Galaxies: general

KW - Supernovae: general

U2 - 10.1093/mnras/sty1581

DO - 10.1093/mnras/sty1581

M3 - Journal article

AN - SCOPUS:85051468179

VL - 479

SP - 3232

EP - 3253

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -

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