output
19912026
Showing 2016 · astro-ph.SRShow all

34 papers · 2 filters

astro-ph.SR2016★ 9 cited

Runaway Dwarf Carbon Stars as Candidate Supernova Ejecta

Kathryn A. Plant, Bruce Margon, Puragra Guhathakurta +3

The dwarf carbon (dC) star SDSS J112801.67+004034.6 has an unusually high radial velocity, 531 km s. We present proper motion and new spectroscopic observations which…

astro-ph.SR2016★ 119 cited

Uniform Atmospheric Retrieval Analysis of Ultracool Dwarfs II: Properties of 11 T-dwarfs

Michael R. Line, Mark S. Marley, Michael C. Liu +7

Brown dwarf spectra are rich in information revealing of the chemical and physical processes operating in their atmospheres. We apply a recently developed atmospheric retrieval too…

astro-ph.SR2016★ 21 cited

Discovery and Follow-up Observations of the Young Type Ia Supernova 2016coj

WeiKang Zheng, Alexei V. Filippenko, Jon Mauerhan +39

The Type~Ia supernova (SN~Ia) 2016coj in NGC 4125 (redshift ) was discovered by the Lick Observatory Supernova Search 4.9 days after the fitted first-light time (FFLT;…

astro-ph.SR2016★ 4 cited

Emission-line stars in M31 from the SPLASH and PHAT surveys

Laura J. Prichard, Puragra Guhathakurta, Katherine M. Hamren +7

We present a sample of 224 stars that emit H (H stars) in the Andromeda galaxy (M31). The stars were selected from 5000 spectra, collected as part of the Spectroscopic…

astro-ph.SR2016★ 31 cited

Convection Destroys the Core/Mantle Structure in Hybrid C/O/Ne White Dwarfs

Jared Brooks, Josiah Schwab, Lars Bildsten +2

A hybrid C/O/Ne white dwarf (WD) -- an unburned C/O core surrounded by an O/Ne/Na mantle -- can be formed if the carbon flame is quenched in a super-AGB (SAGB) star or white dwarf…

astro-ph.SR2016★ 63 cited

The evolution of superluminous supernova LSQ14mo and its interacting host galaxy system

T. -W. Chen, M. Nicholl, S. J. Smartt +26

We present and analyse an extensive dataset of the superluminous supernova (SLSN) LSQ14mo (z = 0.256), consisting of a multi-colour lightcurve from -30 d to +70 d in the rest-frame…

astro-ph.SR2016★ 24 cited

The Candidate Progenitor of the Type IIn SN 2010jl is Not an Optically Luminous Star

Ori D. Fox, Schuyler D. Van Dyk, Eli Dwek +8

The nature of the progenitor star (or system) for the Type IIn supernova (SN) subclass remains uncertain. While there are direct imaging constraints on the progenitors of at least…

astro-ph.SR2016★ 58 cited

On the Progenitor of the Type IIb Supernova 2016gkg

Charles D. Kilpatrick, Ryan J. Foley, Louis E. Abramson +7

We present a detection in pre-explosion Hubble Space Telescope (HST) imaging of a point source consistent with being the progenitor star of the Type IIb supernova (SN IIb) 2016gkg.…

astro-ph.SR2016★ 41 cited

Turbulent transport by diffusive stratified shear flows: from local to global models. Part I: Numerical simulations of a stratified plane Couette flow

P. Garaud, D. Gagnier, J. Verhoeven

Shear-induced turbulence could play a significant role in mixing momentum and chemical species in stellar radiation zones, as discussed by Zahn (1974). In this paper we analyze the…

astro-ph.SR2016★ 29 cited

The effect of rotation on oscillatory double-diffusive convection (semiconvection)

Ryan Moll, Pascale Garaud

Oscillatory double-diffusive convection (ODDC, more traditionally called semiconvection) is a form of linear double-diffusive instability that occurs in fluids that are unstably st…

astro-ph.SR2016★ 46 cited

After the Fall: Late-Time Spectroscopy of Type IIP Supernovae

Jeffrey M. Silverman, Stephanie Pickett, J. Craig Wheeler +11

Herein we analyse late-time (post-plateau; 103 < t < 1229 d) optical spectra of low-redshift (z < 0.016), hydrogen-rich Type IIP supernovae (SNe IIP). Our newly constructed sample…

astro-ph.SR2016★ 169 cited

Systematic non-LTE study of the [Fe/H] F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu

G. Zhao, L. Mashonkina, H. L. Yan +14

For the first time, we present an extensive study of stars with individual non-local thermodynamic equilibrium (NLTE) abundances for 17 chemical elements from Li to Eu in a sample…

astro-ph.SR2016★ 27 cited

A high mass progenitor for the Type Ic Supernova 2007gr inferred from its environment

Justyn Maund, Enrico Ramirez-Ruiz

We present an analysis of late-time Hubble Space Telescope Wide Field Camera 3 and Wide Field Planetary Camera 2 observations of the site of the Type Ic SN 2007gr in NGC 1058. The…

astro-ph.SR2016★ 13 cited

Stellar Flares in the CSTAR Field: Results from the 2008 Data Set

En-Si Liang, Songhu Wang, Ji-Lin Zhou +6

The Chinese Small Telescope ARray (CSTAR) is the first Chinese astronomical instrument placed in Antarctica. It is a group of four identical, fully automatic telesc…

astro-ph.SR2016★ 13 cited

L-band Spectroscopy with Magellan-AO/Clio2: First Results on Young Low-Mass Companions

Jordan M. Stone, Josh Eisner, Andy Skemer +6

L-band spectroscopy is a powerful probe of cool low-gravity atmospheres: The P, Q, and R branch fundamental transitions of methane near 3.3 m provide a sensitive probe of carbon…

astro-ph.SR2016★ 47 cited

Optical Identification of Cepheids in 19 Host Galaxies of Type Ia Supernovae and NGC 4258 with the Hubble Space Telescope

Samantha L. Hoffmann, Lucas M. Macri, Adam G. Riess +10

We present results of an optical search for Cepheid variable stars using the Hubble Space Telescope (HST) in 19 hosts of Type Ia supernovae (SNe Ia) and the maser-host galaxy NGC 4…

astro-ph.SR2016★ 45 cited

Observed Variability at 1um and 4um in the Y0 Brown Dwarf WISEP J173835.52+273258.9

S. K. Leggett, Michael C. Cushing, Kevin K. Hardegree-Ullman +10

We have monitored photometrically the Y0 brown dwarf WISEP J173835.52+273258.9 (W1738) at both near- and mid-infrared wavelengths. This ~1 Gyr-old 400K dwarf is at a distance of 8p…

astro-ph.SR2016★ 8 cited

Optical and ultraviolet spectroscopic analysis of SN 2011fe at late times

Brian Friesen, E. Baron, Jerod T. Parrent +16

We present optical spectra of the nearby Type Ia supernova SN 2011fe at 100, 205, 311, 349, and 578 days post-maximum light, as well as an ultraviolet spectrum obtained with Hubble…

astro-ph.SR2016★ 132 cited

An Unstable Truth: How Massive Stars get their Mass

Anna L. Rosen, Mark R. Krumholz, Christopher F. McKee +1

The pressure exerted by massive stars' radiation fields is an important mechanism regulating their formation. Detailed simulation of massive star formation therefore requires an ac…

astro-ph.SR2016★ 19 cited

The Chemical Composition of Red Giant Branch Stars in the Galactic Globular Clusters NGC 6342 and NGC 6366

Christian I. Johnson, Nelson Caldwell, R. Michael Rich +2

We present radial velocities and chemical abundances for red giant branch stars in the Galactic bulge globular clusters NGC 6342 and NGC 6366. The velocities and abundances are bas…

astro-ph.SR2016★ 53 cited

The First Focused Hard X-ray Images of the Sun with NuSTAR

Brian W. Grefenstette, Lindsay Glesener, Säm Krucker +20

We present results from the the first campaign of dedicated solar observations undertaken by the \textit{Nuclear Spectroscopic Telescope ARray} ({\em NuSTAR}) hard X-ray telescope.…

astro-ph.SR2016★ 20 cited

Time-Varying Sodium Absorption in the Type Ia Supernova 2013gh

R. Ferretti, R. Amanullah, A. Goobar +18

Temporal variability of narrow absorption lines in high-resolution spectra of Type Ia supernovae (SNe Ia) is studied to search for circumstellar matter. Time series which resolve t…

astro-ph.SR2016★ 105 cited

Lessons from the Onset of a Common Envelope Episode: the Remarkable M31 2015 Luminous Red Nova Outburst

Morgan MacLeod, Phillip Macias, Enrico Ramirez-Ruiz +3

This paper investigates the recent stellar merger transient M31LRN 2015 in the Andromeda galaxy. We analyze published optical photometry and spectroscopy along with a Hubble Space…

astro-ph.SR2016★ 87 cited

Evolution of Flare Ribbons, Electric Currents and Quasi-separatrix Layers During an X-class Flare

M. Janvier, A. Savcheva, E. Pariat +6

The standard model for eruptive flares has in the past few years been extended to 3D. It predicts typical J-shaped photospheric footprints of the coronal current layer, forming at…