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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
Spinning Bar and a Star-formation Inefficient Repertoire: Turbulence in Hickson Compact Group NGC 7674
DOI: 10.3847/1538-4357/ab77ae Bibcode: 2020ApJ...893...26S

Kewley, Lisa J.; Federrath, Christoph; Groves, Brent +2 more

The physics regulating star formation (SF) in Hickson Compact Groups (HCG) has thus far been difficult to describe, due to their unique kinematic properties. In this study, we expand upon previous works to devise a more physically meaningful SF relation able to better encompass the physics of these unique systems. We combine CO(1-0) data from the …

2020 The Astrophysical Journal
eHST 7
Heliospheric Maps from Cassini INCA Early in the Cruise to Saturn
DOI: 10.3847/2041-8213/abbd9e Bibcode: 2020ApJ...902L..45W

Mitchell, D. G.; Krimigis, S.; Clark, G. +8 more

We present new energetic neutral atom (ENA) maps from the Ion and Neutral Camera (INCA) instrument on Cassini from the year 2000, prior to Cassini's encounter with Jupiter. These maps are the first produced for the year 2000 and are the only maps with comprehensive spatial coverage from the peak of solar cycle 23. These ENA maps span the energy ra…

2020 The Astrophysical Journal
Cassini 7
Dying of the Light: An X-Ray Fading Cold Quasar at z ∼ 0.405
DOI: 10.3847/1538-4357/abb94a Bibcode: 2020ApJ...903..106C

Kirkpatrick, Allison; Trump, Jonathan R.; LaMassa, Stephanie +11 more

Cold quasars are a rare subpopulation observed to host unobscured, X-ray luminous active galactic nuclei (AGN) while also retaining a cold gas supply fueling high star formation rates. These objects are interpreted as AGN early in their evolution. We present new SOFIA HAWC+ far-infrared observations, far-ultraviolet to far-infrared (FUV-FIR) photo…

2020 The Astrophysical Journal
Herschel XMM-Newton 7