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We investigate how the different types of supernovae are relatively affected by the metallicity of their host galaxy. We match the SAI Supernova Catalog to the SDSS-DR4 catalog of star-forming galaxies with measured metallicities. These…

天体物理学 · 物理学 2010-11-11 Jose L. Prieto , Krzysztof Z. Stanek , John F. Beacom

Type II SNe can trace star formation to probe its global metallicity distribution at low-redshift. We present oxygen and iron abundance distributions of SN II progenitor regions that avoid many previous sources of bias. Because Fe (rather…

宇宙学与河外天体物理 · 物理学 2015-06-05 R. Stoll , J. L. Prieto , K. Z. Stanek , R. W. Pogge

We present the largest spectroscopic study of the host environments of Type Ibc supernovae (SN Ibc) discovered exclusively by untargeted SN searches. Past studies of SN Ibc host environments have been biased towards high-mass,…

Context: Stellar evolution theory suggests that the relationship between number ratios of supernova (SN) types and metallicity holds important clues as to the nature of the progenitor stars (mass, metallicity, rotation, binarity, etc).…

高能天体物理现象 · 物理学 2015-05-13 S. Boissier , N. Prantzos

We analyse 33 Type I superluminous supernovae (SLSNe) taken from ZTF's Bright Transient Survey to investigate the local environments of their host galaxies. We use a spectroscopic sample of galaxies from the SDSS to determine the…

星系天体物理 · 物理学 2023-07-26 Cressida Cleland , Sean L. McGee , Matt Nicholl

Metallicity plays a crucial role in the evolution of massive stars and their final core-collapse supernova (CCSN) explosions. Integral-field-unit (IFU) spectroscopy can provide a spatially resolved view of SN host galaxies and serve as a…

星系天体物理 · 物理学 2025-08-04 Qiang Xi , Ning-Chen Sun , Yi-Han Zhao , Justyn R. Maund , Zexi Niu , Adam J. Singleton , Jifeng Liu

Spectral modelling of SNII atmospheres indicates a clear dependence of metal line strengths on progenitor metallicity. This motivates further work to evaluate the accuracy with which these SNe can be used as metallicity indicators. To…

The efficient use of Type Ia supernovae (SNIa) for cosmological studies requires knowledge of any parameter that can affect their luminosity in either systematic or statistical ways. Observational samples of SNIa commonly use the…

宇宙学与河外天体物理 · 物理学 2015-05-27 Eduardo Bravo , Carles Badenes

This work presents measurements of the local HII environment metallicities of core-collapse supernovae (SNe) within a luminosity distance of 30 Mpc. 76 targets were observed at the Isaac Newton Telescope and environment metallicities could…

星系天体物理 · 物理学 2022-03-29 R. Ganss , J. L. Pledger , A. E. Sansom , P. A. James , J. Puls , S. M. Habergham-Mawson

We use the latest dataset of supernova (SN) host galaxies to investigate how the host properties -- stellar mass, star formation rate, metallicity, absolute magnitude, and colour -- differ across SN types, with redshift-driven selection…

星系天体物理 · 物理学 2024-09-19 Yu-Jing Qin , Ann Zabludoff

Metallicity is expected to influence not only the lives of massive stars but also the outcome of their deaths as supernovae (SNe) and as gamma-ray bursts (GRBs). However, there are surprisingly few direct measurements of the local…

宇宙学与河外天体物理 · 物理学 2011-03-29 Maryam Modjaz , L. Kewley , J. S. Bloom , A. V. Filippenko , D. Perley , J. M. Silverman

We present constraints on the progenitor metallicities of core-collapse supernovae. To date, nearly all metallicity constraints have been inferred from indirect methods such as metallicity gradients in host galaxies, luminosities of host…

宇宙学与河外天体物理 · 物理学 2015-05-19 J. P. Anderson , R. A. Covarrubias , P. A. James , M. Hamuy , S. M. Habergham

The metallicity of the progenitor system producing a type Ia supernova (SN Ia) could play a role in its maximum luminosity, as suggested by theoretical predictions. We present an observational study to investigate if such a relationship…

This work presents measurements of local HII environment metallicities of core-collapse supernovae (SNe) in hosts with redshifts up to z$\sim$0.025. 139 SNe environments were observed at the Isaac Newton Telescope and data of an additional…

星系天体物理 · 物理学 2025-09-09 R. Ganss , J. L. Pledger , A. E. Sansom , P. A. James , J. Puls , S. M. Habergham-Mawson

The origin of the blue supergiant (BSG) progenitor of Supernova (SN) 1987A has long been debated, along with the role that its sub-solar metallicity played. We now have a sample of 1987A-like SNe that arise from the core collapse (CC) of…

宇宙学与河外天体物理 · 物理学 2014-08-26 F. Taddia , J. Sollerman , A. Razza , E. Gafton , A. Pastorello , C. Fransson , M. D. Stritzinger , G. Leloudas , M. Ergon

The effect of progenitor metallicity on Type Ia Supernovae (SNe Ia) has important cosmological implications due to the need for these standardizable candles to be compared across large spans of cosmic time in which the progenitor stars…

星系天体物理 · 物理学 2020-02-19 Peter J. Brown , Nicole R. Crumpler

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…

We study the effect of environment on the properties of type Ia supernovae by analyzing the integrated spectra of 57 local type Ia supernova host galaxies. We deduce from the spectra the metallicity, current star formation rate, and star…

天体物理学 · 物理学 2009-11-13 J. S. Gallagher , P. M. Garnavich , P. Berlind , P. Challis , S. Jha , R. P. Kirshner

We present measurements of the pseudo-equivalent width of the Fe II,$\lambda$5018 absorption feature in the spectra of 12 Type IIP supernovae (SNe II) in low luminosity ($M>-17$) dwarf host galaxies. The Fe II,$\lambda$5018 line has been…

太阳与恒星天体物理 · 物理学 2019-01-16 Spencer Scott , Matt Nicholl , Peter Blanchard , Sebastian Gomez , Edo Berger

Despite the tremendous impact of Type Ia supernovae (SNe Ia) on the field of cosmology, their underlying physics are still poorly understood. Studies have found an intriguing correlation between standardized Type Ia supernova (SN Ia)…

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