Search Publications

Optical Observations Reveal Strong Evidence for High-energy Neutrino Progenitor
DOI: 10.3847/2041-8213/ab96ba Bibcode: 2020ApJ...896L..19L

Rebolo, R.; Buckley, D. A. H.; Böttcher, M. +32 more

We present the earliest astronomical observation of a high-energy neutrino error box of which the variability was discovered after high-energy-neutrino detection. The one robotic telescope of the MASTER global international networks automatically imaged the error box of the very high-energy-neutrino event IceCube-170922A. Observations were carried…

2020 The Astrophysical Journal
Gaia 22
Discovery of a Young Stellar Snake with Two Dissolving Cores in the Solar Neighborhood
DOI: 10.3847/1538-4357/abbf4b Bibcode: 2020ApJ...904..196T

Tian, Hai-Jun

We report the discovery of a young (only 30-40 Myr) snake-like structure (dubbed a stellar snake) in the solar neighborhood from Gaia DR2. The average distance of this structure is about 310 pc from us. Both the length and width are over 200 pc, but the thickness is only about 80 pc. The snake has one tail and two dissolving cores, which can be cl…

2020 The Astrophysical Journal
Gaia 22
IRIS Si IV Line Profiles at Flare Ribbons as Indications of Chromospheric Condensation
DOI: 10.3847/1538-4357/ab9014 Bibcode: 2020ApJ...896..154Y

Ding, M. D.; Li, Y.; Li, D. +3 more

We present temporal variations of the Si IV line profiles at the flare ribbons in three solar flares observed by the Interface Region Imaging Spectrograph. In the M1.1 flare on 2014 September 6 and the X1.6 flare on 2014 September 10, the Si IV line profiles evolve from wholly redshifted to red-wing enhanced with the flare development. However, in…

2020 The Astrophysical Journal
IRIS 22
Nature of Compton-thick Active Galactic Nuclei in "Nonmerging" Luminous Infrared Galaxies UGC 2608 and NGC 5135 Revealed with Broadband X-Ray Spectroscopy
DOI: 10.3847/1538-4357/ab94b1 Bibcode: 2020ApJ...897..107Y

Imanishi, Masatoshi; Tanimoto, Atsushi; Ueda, Yoshihiro +4 more

We have analyzed the broadband X-ray spectra of active galactic nuclei (AGNs) in two "nonmerging" luminous infrared galaxies (LIRGs), UGC 2608 and NGC 5135, utilizing the data of Nuclear Spectroscopic Telescope Array, Suzaku, XMM-Newton, and Chandra. Applying the X-ray clumpy-torus model (XCLUMPY), we find that both sources have similar spectra ch…

2020 The Astrophysical Journal
Suzaku XMM-Newton 22
Lyman Continuum Escape Fraction from Low-mass Starbursts at z = 1.3
DOI: 10.3847/1538-4357/abbd43 Bibcode: 2020ApJ...904...59A

Teplitz, Harry I.; Scarlata, Claudia; Henry, Alaina +8 more

We present a new constraint on the Lyman continuum (LyC) escape fraction at $z\sim 1.3$ . We obtain deep, high sensitivity far-UV imaging with the Advanced Camera for Surveys Solar Blind Channel on the Hubble Space Telescope, targeting 11 star-forming galaxies at 1.2 < z < 1.4. The galaxies are selected from the 3D-HST survey to have high Hα…

2020 The Astrophysical Journal
eHST 22
Is NGC 5824 the Core of the Progenitor of the Cetus Stream?
DOI: 10.3847/1538-4357/abc338 Bibcode: 2020ApJ...905..100C

Zhao, Gang; Zhao, Jing-Kun; Kang, Xi +5 more

The complicated story of the Cetus Stream (CS) is recently revealed by its newly discovered ∼150 members with 6D kinematics from the cross-matched catalog of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) DR5 K giants and Gaia DR2. It exhibits a very diffuse structure at heliocentric distances between 20 and 50 kpc, extendi…

2020 The Astrophysical Journal
Gaia 22
Network Jets as the Driver of Counter-streaming Flows in a Solar Filament/Filament Channel
DOI: 10.3847/2041-8213/ab9ac1 Bibcode: 2020ApJ...897L...2P

Tiwari, Sanjiv K.; Panesar, Navdeep K.; Moore, Ronald L. +1 more

Counter-streaming flows in a small (100″ long) solar filament/filament channel are directly observed in high-resolution Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA) extreme-ultraviolet (EUV) images of a region of enhanced magnetic network. We combine images from SDO/AIA, SDO/Helioseismic and Magnetic Imager (HMI), and the In…

2020 The Astrophysical Journal
IRIS 22
The CGM at Cosmic Noon with KCWI: Outflows from a Star-forming Galaxy at z = 2.071
DOI: 10.3847/1538-4357/abc561 Bibcode: 2020ApJ...904..164N

Kacprzak, Glenn G.; Churchill, Christopher W.; Davé, Romeel +3 more

We present the first results from our "CGM at Cosmic Noon with KCWI" program to study gas flows in the circumgalactic medium (CGM) at z = 2-3. Combining the power of a high-resolution VLT/UVES quasar spectrum, a Hubble Space Telescope/Advanced Camera for Surveys image, and integral field spectroscopy with Keck/KCWI (Keck Cosmic Web Imager), we det…

2020 The Astrophysical Journal
eHST 22
An Observationally Constrained Analytical Model for Predicting the Magnetic Field Vectors of Interplanetary Coronal Mass Ejections at 1 au
DOI: 10.3847/1538-4357/ab5fd7 Bibcode: 2020ApJ...888..121S

Gopalswamy, Nat; Srivastava, Nandita; Sarkar, Ranadeep

We report on an observationally constrained analytical model, the INterplanetary Flux ROpe Simulator (INFROS), for predicting the magnetic field vectors of coronal mass ejections (CMEs) in the interplanetary medium. The main architecture of INFROS involves using the near-Sun flux rope properties obtained from the observational parameters that are …

2020 The Astrophysical Journal
SOHO 22
Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068
DOI: 10.3847/1538-4357/ab8945 Bibcode: 2020ApJ...895...31B

Fox, O. D.; Zhang, X.; Reichart, D. E. +46 more

We present the discovery and high-cadence follow-up observations of SN 2018ivc, an unusual SNe II that exploded in NGC 1068 (D = 10.1 Mpc). The light curve of SN 2018ivc declines piecewise-linearly, changing slope frequently, with four clear slope changes in the first 30 days of evolution. This rapidly changing light curve indicates that interacti…

2020 The Astrophysical Journal
eHST 22