Search Publications

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
The Correlation of Outflow Kinematics with Star Formation Rate. VI. Gas Outflows in AGNs
DOI: 10.3847/1538-4357/abad97 Bibcode: 2020ApJ...901...66W

Rakshit, Suvendu; Woo, Jong-Hak; Son, Donghoon

We investigate the connection between ionized gas outflows and star formation activity using a large sample of type 1 and 2 active galactic nuclei (AGNs) with far-infrared detections or star formation rate (SFR) estimates. The strength of ionized gas outflows, measured by the velocity dispersion and velocity shift of the [O III] emission line, cle…

2020 The Astrophysical Journal
AKARI Herschel 22
The Drivers of Active Region Outflows into the Slow Solar Wind
DOI: 10.3847/1538-4357/ab8a4c Bibcode: 2020ApJ...894..144B

Golub, Leon; Winebarger, Amy R.; Warren, Harry P. +13 more

Plasma outflows from the edges of active regions have been suggested as a possible source of the slow solar wind. Spectroscopic measurements show that these outflows have an enhanced elemental composition, which is a distinct signature of the slow wind. Current spectroscopic observations, however, do not have sufficient spatial resolution to disti…

2020 The Astrophysical Journal
Hinode 22
The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. I. Survey Overview and First Results for Andromeda I
DOI: 10.3847/1538-4357/ab88a2 Bibcode: 2020ApJ...894..135S

Javadi, Atefeh; Saremi, Elham; van Loon, Jacco Th. +10 more

An optical monitoring survey in nearby dwarf galaxies was carried out with the 2.5 m Isaac Newton Telescope. Fifty-five dwarf galaxies and four isolated globular clusters in the Local Group were observed with the Wide Field Camera. The main aims of this survey are to identify the most evolved asymptotic giant branch (AGB) stars and red supergiants…

2020 The Astrophysical Journal
Gaia 21