Type II Supernova Spectral Diversity. II. Spectroscopic and Photometric Correlations
We present an analysis of observed trends and correlations between a large range of spectral and photometric parameters of more than 100 type II supernovae (SNe II), during the photospheric phase. We define a common epoch for all SNe of 50 days post-explosion, where the majority of the sample is lik...
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| Autores principales: | , , , , , , , , , |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2017
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/87146 |
| Aporte de: |
| id |
I19-R120-10915-87146 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Ciencias Astronómicas supernovae: general surveys |
| spellingShingle |
Ciencias Astronómicas supernovae: general surveys Gutiérrez, Claudia P. Anderson, Joseph P. Hamuy, Mario González Gaitan, Santiago Galbany, Lluis Dessart, Luc Stritzinger, Maximilian D. Phillips, Mark M. Morrell, Nidia Irene Folatelli, Gastón Type II Supernova Spectral Diversity. II. Spectroscopic and Photometric Correlations |
| topic_facet |
Ciencias Astronómicas supernovae: general surveys |
| description |
We present an analysis of observed trends and correlations between a large range of spectral and photometric parameters of more than 100 type II supernovae (SNe II), during the photospheric phase. We define a common epoch for all SNe of 50 days post-explosion, where the majority of the sample is likely to be under similar physical conditions. Several correlation matrices are produced to search for interesting trends between more than 30 distinct light-curve and spectral properties that characterize the diversity of SNe II. Overall, SNe with higher expansion velocities are brighter, have more rapidly declining light curves, shorter plateau durations, and higher <sup>56</sup>Ni masses. Using a larger sample than previous studies, we argue that "<i>Pd</i>" - the plateau duration from the transition of the initial to "plateau" decline rates to the end of the "plateau" - is a better indicator of the hydrogen envelope mass than the traditionally used optically thick phase duration (<i>OPTd</i>: explosion epoch to end of plateau). This argument is supported by the fact that <i>Pd</i> also correlates with s<sub>3</sub>, the light-curve decline rate at late times: lower <i>Pd</i> values correlate with larger s<sub>3</sub> decline rates. Large s<sub>3</sub> decline rates are likely related to lower envelope masses, which enables gamma-ray escape. We also find a significant anticorrelation between <i>Pd</i> and s<sub>2</sub> (the plateau decline rate), confirming the long standing hypothesis that faster declining SNe II (SNe IIL) are the result of explosions with lower hydrogen envelope masses and therefore have shorter <i>Pd</i> values. |
| format |
Articulo Articulo |
| author |
Gutiérrez, Claudia P. Anderson, Joseph P. Hamuy, Mario González Gaitan, Santiago Galbany, Lluis Dessart, Luc Stritzinger, Maximilian D. Phillips, Mark M. Morrell, Nidia Irene Folatelli, Gastón |
| author_facet |
Gutiérrez, Claudia P. Anderson, Joseph P. Hamuy, Mario González Gaitan, Santiago Galbany, Lluis Dessart, Luc Stritzinger, Maximilian D. Phillips, Mark M. Morrell, Nidia Irene Folatelli, Gastón |
| author_sort |
Gutiérrez, Claudia P. |
| title |
Type II Supernova Spectral Diversity. II. Spectroscopic and Photometric Correlations |
| title_short |
Type II Supernova Spectral Diversity. II. Spectroscopic and Photometric Correlations |
| title_full |
Type II Supernova Spectral Diversity. II. Spectroscopic and Photometric Correlations |
| title_fullStr |
Type II Supernova Spectral Diversity. II. Spectroscopic and Photometric Correlations |
| title_full_unstemmed |
Type II Supernova Spectral Diversity. II. Spectroscopic and Photometric Correlations |
| title_sort |
type ii supernova spectral diversity. ii. spectroscopic and photometric correlations |
| publishDate |
2017 |
| url |
http://sedici.unlp.edu.ar/handle/10915/87146 |
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