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"High-velocity features" (HVFs) are spectral features in Type Ia supernovae (SNe Ia) that have minima indicating significantly higher (by greater than about 6000 km/s) velocities than typical "photospheric-velocity features" (PVFs). The…

The high-velocity features (HVFs) in optical spectra of type Ia supernovae (SNe Ia) are examined with a large sample including very early-time spectra (e.g., t < -7 days). Multiple Gaussian fits are applied to examine the HVFs and their…

High Energy Astrophysical Phenomena · Physics 2015-09-30 Xulin Zhao , Xiaofeng Wang , Keiichi Maeda , Hanna Sai , Tianmeng Zhang , Jujia Zhang , Fang Huang , Liming Rui , Qi Zhou , Jun Mo

Photospheric and high-velocity features (PVFs and HVFs) of Si II $\lambda$6355 and Ca II IR3 lines in supernova Ia (SN Ia) spectra provide insights into ejecta structure, energetics, and circumstellar interaction, yet their interplay…

Astrophysics of Galaxies · Physics 2026-01-21 A. A. Hakobyan , M. H. Gevorgyan , A. G. Karapetyan , G. A. Mamon , D. Kunth , V. Adibekyan , L. V. Barkhudaryan

We report measurements and analysis of high-velocity (> 20,000 km/s) and photospheric absorption features in a series of spectra of the Type Ia supernova (SN) 2009ig obtained between -14d and +13d with respect to the time of maximum B-band…

Appearing as secondary higher-velocity absorption components, high-velocity features (HVFs) have been observed in several absorption lines in many Type Ia supernovae (SNe Ia). The frequency and ubiquity of these components in silicon and…

We use a sample of 58 low-redshift (z <= 0.03) Type Ia supernovae (SNe Ia) having well-sampled light curves and spectra near maximum light to examine the behaviour of high-velocity features (HVFs) in SN Ia spectra. We take advantage of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Michael J. Childress , Alexei V. Filippenko , Mohan Ganeshalingam , Brian P. Schmidt

High-velocity features (HVF), especially of Ca II, are frequently seen in Type Ia supernova observed prior to B-band maximum (Bmax). These HVF evolve in velocity from more than 25,000 km/s, in the days after first light, to about 18,000…

Solar and Stellar Astrophysics · Physics 2017-12-01 Brian W. Mulligan , J. Craig Wheeler

We present a detailed analysis of spectral line profiles in Type Ia supernova (SN Ia) spectra. We focus on the feature at ~3500 - 4000 A, which is commonly thought to be caused by blueshifted absorption of Ca H&K. Unlike some other spectral…

Solar and Stellar Astrophysics · Physics 2015-06-12 Ryan J. Foley

The absorption feature O I 7773 is an important spectral indicator for type Ia supernovae (SNe~Ia) that can be used to trace the unburned material at outer layers of the exploding white dwarf. In this work, we use a large sample of SNe~Ia…

High Energy Astrophysical Phenomena · Physics 2016-08-08 Xulin Zhao , Keiichi Maeda , Xiaofeng Wang , Lifan Wang , Hanna Sai , Jujia Zhang , Tianmeng Zhang , Fang Huang , Liming Rui

Although type Ia supernovae (SNe Ia) are very useful in many astrophysical fields, their exact nature is still unclear, e.g. the progenitor and explosion models. The high-velocity features (HVFs) in optical spectra of SNe Ia could provide…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Xiangcun Meng

Spectral synthesis in 3-dimensional (3D) space for the earliest spectra of Type Ia supernovae (SNe Ia) is presented. In particular, the high velocity absorption features that are commonly seen at the earliest epochs ($\sim 10$ days before…

Astrophysics · Physics 2009-11-11 Masaomi Tanaka , Paolo A. Mazzali , Keiichi Maeda , Ken'ichi Nomoto

We explore the possible nature of high-velocity features in Type~Ia supernovae by presenting synthetic spectra generated from hydrodynamic models of interaction between the supernova and a compact circumstellar shell. We use TARDIS to…

High Energy Astrophysical Phenomena · Physics 2019-01-30 B. W. Mulligan , K. Zhang , J. C. Wheeler

We present photometry and time-series spectroscopy of the nearby type Ia supernova (SN Ia) SN 2015F over $-16$ days to $+80$ days relative to maximum light, obtained as part of the Public ESO Spectroscopic Survey of Transient Objects…

We present high-resolution (FWHM ~ 0.3-1.5 km/s) spectra of interstellar Ca I absorption toward 30 Galactic stars. Comparisons of the column densities of Ca I, Ca II, K I, and other species -- for individual components identified in the…

Astrophysics · Physics 2009-11-07 Daniel E. Welty , L. M. Hobbs , Donald C. Morton

The type Ia supernova (SN) 2012fr displayed an unusual combination of its Si II {\lambda}{\lambda}5972, 6355 features. This includes the ratio of their pseudo equivalent widths, placing it at the border of the Shallow Silicon (SS) and Core…

We analyse spectroscopic measurements of 122 type Ia supernovae (SNe Ia) with z<0.09 discovered by the Palomar Transient Factory, focusing on the properties of the Si II 6355 and Ca II `near-infrared triplet' absorptions. We examine the…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Y. -C. Pan , M. Sullivan , K. Maguire , A. Gal-Yam , I. M. Hook , D. A. Howell , P. E. Nugent , P. A. Mazzali

The neutral hydrogen and the ionized helium absorption in the spectra of quasars are unique probes of structure in the early universe. We present Far-Ultraviolet Spectroscopic Explorer observations of the line of sight to the quasar…

High-velocity features in Type Ia supernova spectra provide a way to probe the outer layers of these explosions. The maximum-light spectra of the unique Type Ia supernova 2000cx exhibit interesting Ca II features with high-velocity…

Astrophysics · Physics 2009-11-07 R. C. Thomas , David Branch , E. Baron , Ken'ichi Nomoto , Weidong Li , Alexei V. Filippenko

We studied the spectral features of Si II $\lambda\lambda$4130, 5972, 6355 and S II W-trough for a large sample of Type Ia supernovae (SNe Ia). We find that in NV (Normal-Velocity) subclass of SNe Ia, these features tend to reach a maximum…

High Energy Astrophysical Phenomena · Physics 2021-04-08 Xulin Zhao , Keiichi Maeda , Xiaofeng Wang , Hanna Sai
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