Search Publications

Interaction of SN Ib 2004dk with a Previously Expelled Envelope
DOI: 10.3847/1538-4357/ab3e36 Bibcode: 2019ApJ...883..120P

Wheeler, J. Craig; Silverman, Jeffrey M.; Pooley, David +7 more

The interaction between the expanding supernova (SN) ejecta with the circumstellar material (CSM) that was expelled from the progenitor prior to explosion is a long-sought phenomenon, yet observational evidence is scarce. Here we confirm a new example: SN 2004dk, originally a hydrogen-poor, helium-rich Type Ib SN that reappeared as a strong {{H}}α…

2019 The Astrophysical Journal
XMM-Newton 18
Detection and Classification of Supernovae Beyond z ∼ 2 Redshift with the James Webb Space Telescope
DOI: 10.3847/1538-4357/ab0a73 Bibcode: 2019ApJ...874..158R

Vinkó, József; Regős, Enikő

Future time-domain surveys for transient events in the near- and midinfrared bands will significantly extend our understanding about the physics of the early universe. In this paper we study the implications of a deep (∼27 mag), long-term (∼3 yr), observationally inexpensive survey with the James Webb Space Telescope (JWST) within its Continuous V…

2019 The Astrophysical Journal
eHST 18
Spectroscopic and Stereoscopic Observations of the Solar Jets
DOI: 10.3847/1538-4357/ab530c Bibcode: 2019ApJ...887..154L

Feng, Li; Lu, Lei; Gan, Weiqun +3 more

We present a comprehensive study of a series of recurrent jets that occurred at the periphery of the NOAA active region 12114 on 2014 July 7. These jets were found to share the same source region and exhibited rotational motions as they propagated outward. The multiwavelength imaging observations made by the AIA and IRIS telescopes reveal that som…

2019 The Astrophysical Journal
IRIS 18
The Role of Clathrate Formation in Europa’s Ocean Composition
DOI: 10.3847/1538-4357/ab40b0 Bibcode: 2019ApJ...885...14B

Mousis, Olivier; Bouquet, Alexis; Danger, Grégoire +2 more

We use a thermodynamic statistical model to evaluate how the composition of Europa’s internal ocean may have been affected by clathrate hydrate formation. Assuming an input of the observed O2 and CO2 from the surface into a mildly acidic ocean (pH < 6), and considering the possibility of contributions by reduced (with CH

2019 The Astrophysical Journal
Rosetta 18
Origin of a Massive Hyper-runaway Subgiant Star LAMOST-HVS1: Implication from Gaia and Follow-up Spectroscopy
DOI: 10.3847/1538-4357/ab05c8 Bibcode: 2019ApJ...873..116H

Mahler, Guillaume; Hattori, Kohei; Castro, Norberto +3 more

We report that LAMOST-HVS1 is a massive hyper-runaway subgiant star with a mass of 8.3 {M} and super-solar metallicity, which was ejected from the inner stellar disk of the Milky Way ∼33 {Myr} ago with the intrinsic ejection velocity of {568}-17+19 {km} {{{s}}}-1 (corrected for the streaming motion of …

2019 The Astrophysical Journal
Gaia 18
Evolution of the Coronal Cavity From the Quiescent to Eruptive Phase Associated with Coronal Mass Ejection
DOI: 10.3847/1538-4357/ab11c5 Bibcode: 2019ApJ...875..101S

West, Matthew J.; Srivastava, Nandita; Mierla, Marilena +2 more

We present the evolution of a coronal cavity encompassing its quiescent and eruptive phases in the lower corona. Using multiple vantage-point observations from the SDO/AIA, STEREO SECCHI/EUVI, and PROBA2/Sun Watcher with the APS and Image Processing (SWAP) extreme ultraviolet (EUV) imagers, we capture a sequence of quasi-static equilibria of the q…

2019 The Astrophysical Journal
PROBA-2 SOHO 18
Automated Swirl Detection Algorithm (ASDA) and Its Application to Simulation and Observational Data
DOI: 10.3847/1538-4357/aabd34 Bibcode: 2019ApJ...872...22L

Liu, Jiajia; Erdélyi, Robertus; Nelson, Chris J.

Swirling motions in the solar atmosphere have been widely observed in recent years and suggested to play a key role in channeling energy from the photosphere into the corona. Here, we present a newly developed Automated Swirl Detection Algorithm (ASDA) and discuss its applications. ASDA is found to be very proficient at detecting swirls in a varie…

2019 The Astrophysical Journal
Hinode 18
2D Isotropic Feature of Solar Wind Turbulence as Shown by Self-correlation Level Contours at Hour Timescales
DOI: 10.3847/1538-4357/aaf64f Bibcode: 2019ApJ...871...93W

He, Jiansen; Wang, Xin; Tu, Chuanyi

The slow wind anisotropy is observed by Dasso et al. as elongation along the magnetic field direction in the magnetic self-correlation contours calculated from data sets of two-day-long data and averaged for five years in 1998-2002, which is consistent with prediction by the “critical balance cascade theory.” More pronounced elongation at smaller …

2019 The Astrophysical Journal
Ulysses 18
Three-dimensional Density Structure of a Solar Coronal Streamer Observed by SOHO/LASCO and STEREO/COR2 in Quadrature
DOI: 10.3847/1538-4357/ab3b58 Bibcode: 2019ApJ...883..152D

Van Doorsselaere, Tom; Zhukov, Andrei N.; Decraemer, Bieke

Helmet streamers are a prominent manifestation of magnetic structures with current sheets in the solar corona. These large-scale structures are regions with high plasma density, overlying active regions and filament channels. We investigate the three-dimensional (3D) structure of a coronal streamer, observed simultaneously by white-light coronagra…

2019 The Astrophysical Journal
SOHO 18
{k}_{\perp }^{-8/3} Spectrum in Kinetic Alfvén Wave Turbulence: Implications for the Solar Wind
DOI: 10.3847/2041-8213/ab2fe6 Bibcode: 2019ApJ...880L..10D

David, Vincent; Galtier, Sébastien

The nature of solar wind turbulence at large scale is rather well understood in the theoretical framework of magnetohydrodynamics. The situation is quite different at subproton scales where the magnetic energy spectrum measured by different spacecraft does not fit with the classical turbulence predictions: a power-law index close to -8/3 is genera…

2019 The Astrophysical Journal
Cluster 18