output
19912026
Showing 2018 · astro-ph.SRShow all

36 papers · 2 filters

astro-ph.SR2018★ 37 cited

Enhanced mixing in magnetized fingering convection, and implications for RGB stars

Peter Harrington, Pascale Garaud

Double-diffusive convection has been well studied in geophysical contexts, but detailed investigations of the regimes characteristic of stellar or planetary interiors have only rec…

astro-ph.SR2018★ 39 cited

Cloud Atlas: Hubble Space Telescope Near-Infrared Spectral Library of Brown Dwarfs, Planetary-mass companions, and hot Jupiters

Elena Manjavacas, Daniel Apai, Yifan Zhou +12

Bayesian atmospheric retrieval tools can place constraints on the properties of brown dwarfs and hot Jupiters atmospheres. To fully exploit these methods, high signal-to-noise spec…

astro-ph.SR2018★ 136 cited

Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime

J. Davy Kirkpatrick, Emily C. Martin, Richard L. Smart +16

We present preliminary trigonometric parallaxes of 184 late-T and Y dwarfs using observations from Spitzer (143), USNO (18), NTT (14), and UKIRT (9). To complete the 20-pc census o…

astro-ph.SR2018★ 25 cited

Joint X-ray, EUV and UV Observations of a Small Microflare

Iain G. Hannah, Lucia Kleint, Säm Krucker +5

We present the first joint observation of a small microflare in X-rays with the Nuclear Spectroscopic Telescope ARray (NuSTAR), UV with the Interface Region Imaging Spectrograph (I…

astro-ph.SR2018★ 26 cited

The long-term evolution and appearance of Type Iax postgenitor stars

Michael Zhang, Jim Fuller, Josiah Schwab +1

Type Iax supernovae may arise from failed explosions of white dwarfs that leave behind a bound remnant (i.e., a "postgenitor" star) that could be identified in wide field surveys.…

astro-ph.SR2018★ 27 cited

Stellar activity analysis of Barnard's Star: Very slow rotation and evidence for long-term activity cycle

B. Toledo-Padrón, J. I. González Hernández, C. Rodríguez-López +58

The search for Earth-like planets around late-type stars using ultra-stable spectrographs requires a very precise characterization of the stellar activity and the magnetic cycle of…

astro-ph.SR2018★ 85 cited

Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the 2 Observations

W. Li, X. Wang, J. Vinkó +160

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the field. The data revealed an excess emission…

astro-ph.SR2018★ 39 cited

Convective overshooting and penetration in a Boussinesq spherical shell

Lydia Korre, Pascale Garaud, Nicholas Brummell

We study the dynamics associated with the extension of turbulent convective motions from a convection zone (CZ) into a stable region (RZ) that lies below the latter. For that purpo…

astro-ph.SR2018★ 93 cited

The Berkeley Sample of Stripped-Envelope Supernovae

Isaac Shivvers, Alexei V. Filippenko, Jeffrey M. Silverman +22

We present the complete sample of stripped-envelope supernova (SN) spectra observed by the Lick Observatory Supernova Search (LOSS) collaboration over the last three decades: 888 s…

astro-ph.SR2018★ 21 cited

Residual Carbon in Oxygen-Neon White Dwarfs and its Implications for Accretion-Induced Collapse

Josiah Schwab, Kyle Akira Rocha

We explore the effects of the residual present in oxygen-neon white dwarfs (ONe WDs) on their evolution towards accretion-induced collapse (AIC). We produce a set…

astro-ph.SR2018★ 8 cited

Mixing via Thermocompositional Convection in Hybrid C/O/Ne White Dwarfs

Josiah Schwab, Pascale Garaud

Convective overshooting in super asymptotic giant branch stars has been suggested to lead to the formation of hybrid white dwarfs with carbon-oxygen cores and oxygen-neon mantles.…

astro-ph.SR2018★ 25 cited

The direct detection of the irradiated brown dwarf in the white dwarf - brown dwarf binary SDSS J141126.20+200911.1

S. L. Casewell, S. P. Littlefair, S. G. Parsons +3

We have observed the eclipsing, post-common envelope white dwarf-brown dwarf binary, SDSS141126.20+200911.1, in the near-IR with the HAWK-I imager, and present here the first direc…

astro-ph.SR2018★ 324 cited

The White Dwarf Initial-Final Mass Relation for Progenitor Stars From 0.85 to 7.5 M

Jeffrey D. Cummings, Jason S. Kalirai, P. -E. Tremblay +2

We present the initial-final mass relation (IFMR) based on the self-consistent analysis of Sirius B and 79 white dwarfs from 13 star clusters. We have also acquired additional sign…

astro-ph.SR2018★ 14 cited

Minimum Orbital Period of Pre-Cataclysmic Variables

L. Nelson, J. Schwab, M. Ristic +1

More than 20 pre-cataclysmic variable (pre-CV) systems have now been discovered with very short orbital periods ranging from 250 min down to 68 min. A pre-CV consists of a white dw…

astro-ph.SR2018★ 46 cited

A Potential Progenitor for the Type Ic Supernova 2017ein

Charles D. Kilpatrick, Tyler Takaro, Ryan J. Foley +9

We report the first detection of a credible progenitor system for a Type Ic supernova (SN Ic), SN 2017ein. We present spectra and photometry of the SN, finding it to be similar to…

astro-ph.SR2018★ 20 cited

Hard X-Ray Constraints on Small-Scale Coronal Heating Events

Andrew J. Marsh, David M. Smith, Lindsay Glesener +7

Much evidence suggests that the solar corona is heated impulsively, meaning that nanoflares may be ubiquitous in quiet and active regions (ARs). Hard X-ray (HXR) observations with…

astro-ph.SR2018★ 61 cited

SN 2017ens: The Metamorphosis of a Luminous Broad-lined Type Ic Supernova into an SN IIn

T. -W. Chen, C. Inserra, M. Fraser +46

We present observations of supernova (SN) 2017ens, discovered by the ATLAS survey and identified as a hot blue object through the GREAT program. The redshift z=0.1086 implies a pea…

astro-ph.SR2018★ 50 cited

Dynamical Masses of Eps Ind B and C: Two Massive Brown Dwarfs at the Edge of the Stellar-Substellar Boundary

Sergio B. Dieterich, Alycia J. Weinberger, Alan P. Boss +6

We report individual dynamical masses for the brown dwarfs Epsilon Indi B and C, which have spectral types of T1.5 and T6, respectively, measured from astrometric orbit mapping. Ou…

astro-ph.SR2018★ 19 cited

Ensemble Properties of the White Dwarf Population of the Old, Solar Metallicity Open Star Cluster Messier 67

Kurtis A. Williams, Paul A. Canton, A. Bellini +4

White dwarfs are excellent forensic tools for studying end-of-life issues surrounding low- and intermediate-mass stars, and the old, solar-metallicity open star cluster Messier 67…

astro-ph.SR2018★ 16 cited

The TRENDS High-Contrast Imaging Survey. VII. Discovery of a Nearby Sirius-like White Dwarf System (HD 169889)

Justin R. Crepp, Erica J. Gonzales, Brendan P. Bowler +8

Monitoring the long-term radial velocity (RV) and acceleration of nearby stars has proven an effective method for directly detecting binary and substellar companions. Some fraction…

astro-ph.SR2018★ 1 cited

Wolf 1465: Not a Bright Dwarf Carbon Star

Bruce Margon, Georgios Dimitriadis

Wolf 1465 has been suggested as a candidate for a bright dwarf carbon star. It is not.

astro-ph.SR2018★ 70 cited

The Dusty Progenitor Star of the Type II Supernova 2017eaw

Charles D. Kilpatrick, Ryan J. Foley

We present pre-explosion photometry of the likely progenitor star of the Type II supernova (SN II) 2017eaw in NGC 6946. We use a Hubble Space Telescope (HST) image of SN 2017eaw to…

astro-ph.SR2018★ 11 cited

The Rise of a Magnetic Flux Tube in a Background Field: Solar Helicity Selection Rules

Bhishek Manek, Nicholas Brummell, Dongwook Lee

The buoyant transport of magnetic fields from the solar interior towards the surface plays an important role in the emergence of active regions, the formation of sunspots and the o…

astro-ph.SR2018★ 27 cited

The effect of rotation on fingering convection in stellar interiors

S. Sengupta, P. Garaud

We study the effects of rotation on the growth and saturation of the double-diffusive fingering (thermohaline) instability at low Prandtl number. Using direct numerical simulations…