Search Publications

A Dust Trap in the Young Multiple System HD 34700
DOI: 10.3847/1538-4357/abc74b Bibcode: 2020ApJ...905..120B

Wilner, David J.; Zhang, Qizhou; Rich, Evan A. +6 more

Millimeter observations of disks around young stars reveal substructures indicative of gas pressure traps that may aid grain growth and planet formation. We present Submillimeter Array observations of HD 34700: two Herbig Ae stars in a close binary system (Aa/Ab, ∼0.25 au), surrounded by a disk presenting a large cavity and spiral arms seen in sca…

2020 The Astrophysical Journal
Gaia 7
Identification of Two Distinct Electron Populations in an Impulsive Solar Energetic Electron Event
DOI: 10.3847/2041-8213/abb098 Bibcode: 2020ApJ...900L..16L

Wang, L.; Zhao, L.; Li, G. +2 more

We examine the release times of energetic electrons in the 2001 April 25 event. An M2.7 flare occurred on 2001 April 25, from AR 09433, located at N18W09. The flare was observed in X-rays by GOES and the Yohkoh spacecraft. The Yohkoh observation also included hard X-ray (HXR) images for all four energy channels: L, M1, M2, and H. We use Yohkoh obs…

2020 The Astrophysical Journal
SOHO 7
Comparing Observed Stellar Kinematics and Surface Densities in a Low-latitude Bulge Field to Galactic Population Synthesis Models
DOI: 10.3847/1538-4357/ab629b Bibcode: 2020ApJ...889..126T

Anderson, Jay; Penny, Matthew T.; Bennett, David P. +3 more

We present an analysis of Galactic bulge stars from Hubble Space Telescope Wide Field Camera 3 observations of the Stanek window (l, b = [0.25, -2.15]) from two epochs approximately two years apart. This data set is adjacent to the provisional Wide-field Infrared Survey Telescope (WFIRST) microlensing field. Proper motions are measured for approxi…

2020 The Astrophysical Journal
Gaia eHST 7
What Determines Solar Flares Producing Interplanetary Type III Radio Bursts?
DOI: 10.3847/2041-8213/aba362 Bibcode: 2020ApJ...898L..24K

Liu, Y.; Cheng, X.; Ding, M. D. +4 more

Energetic electrons accelerated by solar flares often give rise to type III radio bursts at a broad wave band and even interplanetary type III bursts (IT3) if the wavelength extends to a decameter-kilometer. In this Letter, we investigate the probability of the flares that produce IT3, based on the sample of 2272 flares above M-class observed from…

2020 The Astrophysical Journal
SOHO 7
Magnetic Connectivity between the Light Bridge and Penumbra in a Sunspot
DOI: 10.3847/2041-8213/ab7dc4 Bibcode: 2020ApJ...893L...2F

Feng, Song; Nakariakov, Valery M.; Yuan, Ding +2 more

A light bridge is a prominent structure commonly observed within a sunspot. Its presence usually triggers a wealth of dynamics in a sunspot and has a lasting impact on sunspot evolution. However, the fundamental structure of light bridges is still not well understood. In this study, we used the high-resolution spectropolarimetry data obtained by t…

2020 The Astrophysical Journal
Hinode 7
A Multiwavelength Study of PSR J1119-6127 after 2016 Outburst
DOI: 10.3847/1538-4357/abb3c4 Bibcode: 2020ApJ...902...96W

Takata, J.; Wang, H. -H.; Dai, S. +4 more

The high magnetic field pulsar PSR J1119-6127, detected from radio to high-energy wavelengths, underwent a magnetar-like outburst beginning on 2016 July 27. In this paper, we study the postoutburst multiwavelength properties of this pulsar from the radio to GeV bands and discuss its similarity with the outburst of the magnetar XTE J1810-197. In ph…

2020 The Astrophysical Journal
XMM-Newton 7
Active-region Tilt Angles from White-light Images and Magnetograms: The Role of Magnetic Tongues
DOI: 10.3847/1538-4357/ab8944 Bibcode: 2020ApJ...894..131P

Démoulin, Pascal; Mandrini, Cristina H.; Poisson, Mariano +1 more

The presence of elongations in active-region (AR) polarities, called magnetic tongues, is mostly visible during their emergence phase. AR tilts have been measured thoroughly using long-term white-light (WL) databases, sometimes combined with magnetic-field information. Since the influence of magnetic tongues on WL tilt measurements has not been ta…

2020 The Astrophysical Journal
SOHO 7
Distortion of Magnetic Fields in BHR 71
DOI: 10.3847/1538-4357/ab7b68 Bibcode: 2020ApJ...892..128K

Kwon, Jungmi; Nagata, Tetsuya; Tamura, Motohide +9 more

The magnetic field structure of a star-forming Bok globule BHR 71 was determined based on near-infrared polarimetric observations of background stars. The magnetic field in BHR 71 was mapped from 25 stars. By using a simple 2D parabolic function, the plane-of-sky magnetic axis of the core was found to be θmag = 125° ± 11°. The plane-of-…

2020 The Astrophysical Journal
Herschel 7
A Survey for C II Emission-line Stars in the Large Magellanic Cloud
DOI: 10.3847/1538-4357/ab9abe Bibcode: 2020ApJ...898...85M

Massey, Philip; Morrell, Nidia; Neugent, Kathryn F. +1 more

We present a narrowband imaging survey of the Large Magellanic Cloud (LMC), designed to isolate the C II λλ7231, 7236 emission lines in objects as faint as mλ7400 ∼ 18. The work is motivated by the recent serendipitous discovery in the LMC of the first confirmed extragalactic [WC11] star, whose spectrum is dominated by C II emission, an…

2020 The Astrophysical Journal
Gaia XMM-Newton 7
Time-domain Study of the Young Massive Cluster Westerlund 2 with the Hubble Space Telescope. I
DOI: 10.3847/1538-4357/ab7372 Bibcode: 2020ApJ...891..182S

Anderson, J.; Lennon, D. J.; Bastian, N. +8 more

Time-domain studies of pre-main-sequence (PMS) stars have long been used to investigate star properties during their early evolutionary phases and to trace the evolution of circumstellar environments. Historically these studies have been confined to the nearest, low-density, star-forming regions. We used the Wide Field Camera 3 on board the Hubble…

2020 The Astrophysical Journal
Gaia eHST 7