Search Publications

Plasma Interactions with the Space Environment in the Acceleration Region: Indications of CME-trailing Reconnection Regions
DOI: 10.3847/1538-4357/aac5dd Bibcode: 2018ApJ...861..118J

Vilas, Faith; Heiles, Carl; Kepley, Amanda A. +6 more

Coronal mass ejections (CMEs) are sources of major geomagnetic disturbances. On 2013 May 10, a CME crossed the signal path between the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft and Earth. Using the MESSENGER signal, characteristics of the density, velocity, and magnetic field properties of the crossing pl…

2018 The Astrophysical Journal
SOHO 11
An Extreme-ultraviolet Wave Generating Upward Secondary Waves in a Streamer-like Solar Structure
DOI: 10.3847/2041-8213/aabe87 Bibcode: 2018ApJ...858L...1Z

Chen, Yao; Feng, Shiwei; Zheng, Ruisheng +2 more

Extreme-ultraviolet (EUV) waves, spectacular horizontally propagating disturbances in the low solar corona, always trigger horizontal secondary waves (SWs) when they encounter the ambient coronal structure. We present the first example of upward SWs in a streamer-like structure after the passing of an EUV wave. This event occurred on 2017 June 1. …

2018 The Astrophysical Journal
SOHO 11
Optical Observations of the Young Type Ic Supernova SN 2014L in M99
DOI: 10.3847/1538-4357/aaceaf Bibcode: 2018ApJ...863..109Z

Zhang, Yu; Wang, Lifan; Wheeler, J. Craig +22 more

We present optical spectroscopic and photometric observations of the nearby type Ic supernova (SN Ic) SN 2014L. This SN was discovered by the Tsinghua-NAOC Transient Survey (TNTS) in the nearby type-Sc spiral galaxy M99 (NGC 4254). Fitting to the early-time light curve indicates that SN 2014L was detected at only a few hours after the shock breako…

2018 The Astrophysical Journal
eHST 11
Toward the Measurement of the Mass of Isolated Neutron Stars: Prediction of Future Astrometric Microlensing Events by Pulsars
DOI: 10.3847/1538-4357/aadfeb Bibcode: 2018ApJ...866..144O

Ofek, Eran O.

The mass of single neutron stars (NSs) can be measured using astrometric microlensing events. In such events, the center-of-light motion of a star lensed by an NS will deviate from the expected nonlensed motion and this deviation can be used to measure the mass of the NS. I search for future conjunctions between pulsars, with measured proper motio…

2018 The Astrophysical Journal
Gaia 11
Observations of Upward Propagating Waves in the Transition Region and Corona above Sunspots
DOI: 10.3847/1538-4357/aaab5a Bibcode: 2018ApJ...855...65H

Fu, Hui; Li, Bo; Xia, Lidong +2 more

We present observations of persistent oscillations of some bright features in the upper-chromosphere/transition region above sunspots taken by IRIS SJ 1400 Å and upward propagating quasi-periodic disturbances along coronal loops rooted in the same region taken by the AIA 171 Å passband. The oscillations of the features are cyclic oscillatory motio…

2018 The Astrophysical Journal
IRIS 11
EPIC 203868608: A Low-mass Quadruple Star System in the Upper Scorpius OB Association
DOI: 10.3847/1538-4357/aadee8 Bibcode: 2018ApJ...865..141W

Albrecht, Simon; Hillenbrand, Lynne A.; Mawet, Dimitri +3 more

Young multiple star systems provide excellent testing grounds for theories of star formation and evolution. EPIC 203868608 was previously studied as a triple star system in the Upper Scorpius OB association, but the followup Keck NIRC2/HIRES/NIRSPAO observations reported here reveal its quadruple nature. We find that the system consists of a doubl…

2018 The Astrophysical Journal
Gaia 11
Size-Luminosity Scaling Relations of Local and Distant Star-forming Regions
DOI: 10.3847/1538-4357/aaeb8f Bibcode: 2018ApJ...869...11C

Do, Tuan; Armus, Lee; Larkin, James E. +8 more

We investigate star-forming scaling relations using Bayesian inference on a comprehensive data sample of low- (z < 0.1) and high-redshift (1 < z < 5) star-forming regions. This full data set spans a wide range of host galaxy stellar mass (M * ∼ 106-1011 {M}) and clump star formation rates (SFR…

2018 The Astrophysical Journal
eHST 11
Discovery of an Active Intermediate-mass Black Hole Candidate in the Barred Bulgeless Galaxy NGC 3319
DOI: 10.3847/1538-4357/aaeb90 Bibcode: 2018ApJ...869...49J

Shu, Xinwen; Zhou, Hongyan; Jiang, Ning +7 more

We report the discovery of an active intermediate-mass black hole (IMBH) candidate in the center of nearby barred bulgeless galaxy NGC 3319. The point X-ray source revealed by archival Chandra and XMM-Newton observations is spatially coincident with the optical and UV galactic nuclei from Hubble Space Telescope observations. The spectral energy di…

2018 The Astrophysical Journal
XMM-Newton eHST 11
Measuring the Local ISM along the Sight Lines of the Two Voyager Spacecraft with HST/STIS
DOI: 10.3847/1538-4357/aac017 Bibcode: 2018ApJ...859...42Z

Redfield, Seth; Wood, Brian E.; Linsky, Jeffrey L. +1 more

In 2012 August, Voyager 1 crossed the heliopause, becoming the first human-made object to exit the solar system. This milestone signifies the beginning of an important new era for local interstellar medium (LISM) exploration. We present measurements of the structure and composition of the LISM in the immediate path of the Voyager spacecraft by usi…

2018 The Astrophysical Journal
eHST 10
Large-amplitude Rapid X-Ray Variability in the Narrow-line Seyfert 1 Galaxy PG 1404+226
DOI: 10.3847/1538-4357/aad193 Bibcode: 2018ApJ...863..178M

Dewangan, G. C.; Mallick, L.

We present the first results from a detailed analysis of a new, long (∼100 ks) XMM-Newton observation of the narrow-line Seyfert 1 galaxy PG 1404+226, which showed a large-amplitude, rapid X-ray variability by a factor of ∼7 in ∼10 ks with an exponential rise and a sharp fall in the count rate. We investigate the origin of the soft X-ray excess em…

2018 The Astrophysical Journal
XMM-Newton 10