Search Publications

Calibrating Star Formation Rate Prescriptions at Different Scales (10 pc-1 kpc) in M31
DOI: 10.3847/1538-4357/ab03ce Bibcode: 2019ApJ...873....3T

Schinnerer, Eva; Blanc, Guillermo A.; Kreckel, Kathryn +9 more

We calibrate commonly used star formation rate (SFR) prescriptions using observations in five kiloparsec-sized fields in the nearby galaxy Andromeda (M31) at 10 pc spatial resolution. Our observations at different scales enable us to resolve the star-forming regions and to distinguish them from non-star-forming components. We use extinction-correc…

2019 The Astrophysical Journal
Herschel 14
The MASSIVE Survey XIII. Spatially Resolved Stellar Kinematics in the Central 1 kpc of 20 Massive Elliptical Galaxies with the GMOS-North Integral Field Spectrograph
DOI: 10.3847/1538-4357/ab1f04 Bibcode: 2019ApJ...878...57E

Ma, Chung-Pei; Greene, Jenny E.; Blakeslee, John P. +5 more

We use observations from the GEMINI-N/GMOS integral field spectrograph (IFS) to obtain spatially resolved stellar kinematics of the central ∼1 kpc of 20 early-type galaxies (ETGs) with stellar masses greater than 1011.7 M in the MASSIVE survey. Together with observations from the wide-field Mitchell IFS at McDonald Observat…

2019 The Astrophysical Journal
eHST 14
Discovery of a Lyα-emitting Dark Cloud within the z ∼ 2.8 SMM J02399-0136 System
DOI: 10.3847/1538-4357/ab0e6f Bibcode: 2019ApJ...875..130L

Ivison, R. J.; Prochaska, J. Xavier; Cai, Zheng +9 more

We present Keck/Keck Cosmic Web Imager (KCWI) integral field spectrograph observations of the complex system surrounding SMM J02399-0136 (a lensed z = 2.8 sub-mm galaxy), including an associated Lyα nebula, a dust-obscured, broad-absorption-line quasar, and neighboring galaxies. At a 3σ surface brightness contour of 1.6 × 10-17 erg s

2019 The Astrophysical Journal
eHST 14
Dynamic Processes of the Moreton Wave on 2014 March 29
DOI: 10.3847/1538-4357/ab3a35 Bibcode: 2019ApJ...883...32C

Shibata, Kazunari; Ichimoto, Kiyoshi; Asai, Ayumi +4 more

On 2014 March 29, an intense solar flare classified as X1.0 occurred in active region 12017. Several associated phenomena accompanied this event, among them a fast-filament eruption, large-scale propagating disturbances in the corona and the chromosphere including a Moreton wave, and a coronal mass ejection. This flare was successfully detected in…

2019 The Astrophysical Journal
Hinode 14
Spectroscopic Constraints on the Cross-sectional Asymmetry and Expansion of Active Region Loops
DOI: 10.3847/1538-4357/ab449e Bibcode: 2019ApJ...885....7K

Young, P. R.; Klimchuk, J. A.; DeForest, C. E. +1 more

We explore the constraints that can be placed on the dimensions of coronal loops out of the plane of the sky by utilizing spectroscopic observations from the Hinode/EUV Imaging Spectrometer (EIS). The usual assumption is that loop cross sections are circular. Changes in intensity are assumed to be the result of changing density, filling factor, an…

2019 The Astrophysical Journal
Hinode 14
ALMA Reveals a Gas-rich, Maximum Starburst in the Hyperluminous, Dust-obscured Quasar W0533-3401 at z ∼ 2.9
DOI: 10.3847/1538-4357/ab5059 Bibcode: 2019ApJ...887...74F

Knudsen, Kirsten K.; Fan, Lulu; Han, Yunkun +1 more

We present ALMA observations and multiwavelength spectral energy distribution analysis in a Wide-field Infrared Survey Explorer-selected, hyperluminous dust-obscured quasar W0533-3401 at z = 2.9. We derive the physical properties of each of its components, such as molecular gas, stars, dust, and the central supermassive black hole (SMBH). Both the…

2019 The Astrophysical Journal
Herschel 14
Multiple Magnetic Reconnections Driven by a Large-scale Magnetic Flux Rope
DOI: 10.3847/1538-4357/ab01cf Bibcode: 2019ApJ...873...23Z

Wang, J. X.; Tan, B. L.; Zhou, G. P. +4 more

Magnetic flux ropes (MFRs), as the most probable core structure of solar eruptive activity, remain mysterious on their origination, magnetic environment, and erupting mechanisms. Here, we newly identify a large-scale hot channel MFR, named “MFR3”, that connects an anti-Hale active region (AR) 11429 and a normal AR 11430 on 2012 March 7 based on mu…

2019 The Astrophysical Journal
SOHO 14
Probing the Innermost Ejecta Layers in Supernova Remnant Kes 75: Implications for the Supernova Progenitor
DOI: 10.3847/2041-8213/ab237c Bibcode: 2019ApJ...878L..19T

Gelfand, Joseph D.; Temim, Tea; Koo, Bon-Chul +3 more

Supernova remnants (SNRs) that contain pulsar wind nebulae (PWNe) are characterized by distinct evolutionary stages. In very young systems, the PWN drives a shock into the innermost supernova (SN) material, giving rise to low-excitation lines and an infrared (IR) continuum from heated dust grains. These observational signatures make it possible to…

2019 The Astrophysical Journal
Herschel 14
Exceptional Extended Field-of-view Observations by PROBA2/SWAP on 2017 April 1 and 3
DOI: 10.3847/1538-4357/ab3b08 Bibcode: 2019ApJ...883...59O

West, Matthew J.; Mierla, Marilena; D'Huys, Elke +2 more

On 2017 April 1 and 3, two large eruptions on the western solar limb, which were associated with M4.4- and M5.8-class flares, respectively, were observed with the Sun Watcher with Active Pixels and Image Processing (SWAP) Extreme Ultraviolet (EUV) solar telescope on board the Project for On Board Autonomy 2 (PROBA2) spacecraft. The large field-of-…

2019 The Astrophysical Journal
PROBA-2 SOHO 14
Broadband X-Ray Spectral and Timing Analyses of the Black Hole Binary Candidate Swift J1658.2-4242: Rapid Flux Variation and the Turn-on of a Transient QPO
DOI: 10.3847/1538-4357/ab24bf Bibcode: 2019ApJ...879...93X

Gandhi, Poshak; Walton, Dominic J.; Miller, Jon M. +6 more

We report results from joint Nuclear Spectroscopic Telescope Array, Swift, and XMM-Newton observations of the newly discovered black hole X-ray binary candidate Swift J1658.2-4242 in the intermediate state. We observe a peculiar event in this source, with its X-ray flux rapidly decreasing by ∼45% in ∼40 s, accompanied by only subtle changes in the…

2019 The Astrophysical Journal
XMM-Newton 14