Search Publications

An Exceptional Dimming Event for a Massive, Cool Supergiant in M51
DOI: 10.3847/1538-4357/ac626c Bibcode: 2022ApJ...930...81J

Smith, Nathan; Strader, Jay; Sand, David J. +6 more

We present the discovery of an exceptional dimming event in a cool supergiant star in the Local Volume spiral M51. The star, dubbed M51-DS1, was found as part of a Hubble Space Telescope (HST) search for failed supernovae (SNe). The supergiant, which is plausibly associated with a very young (≲6 Myr) stellar population, showed clear variability (a…

2022 The Astrophysical Journal
eHST 12
A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers during the Third Gravitational-wave Observing Run
DOI: 10.3847/1538-4357/ac4d34 Bibcode: 2022ApJ...927...50R

Fong, W.; Sand, D. J.; Rastinejad, J. C. +9 more

We present a comprehensive analysis of 653 optical candidate counterparts reported during the third gravitational-wave (GW) observing run. Our sample concentrates on candidates from the 15 events (published in GWTC-2, GWTC-3, or not retracted on GraceDB) that had a >1% chance of including a neutron star in order to assess their viability as tru…

2022 The Astrophysical Journal
Gaia 12
Coronal Mass Ejections and Type II Radio Emission Variability during a Magnetic Cycle on the Solar-type Star ϵ Eridani
DOI: 10.3847/1538-4357/ac35de Bibcode: 2022ApJ...924..115O

Ó Fionnagáin, Dúalta; Kavanagh, Robert D.; Vidotto, Aline A. +5 more

We simulate possible stellar coronal mass ejection (CME) scenarios over the magnetic cycle of ϵ Eridani (18 Eridani; HD 22049). We use three separate epochs from 2008, 2011, and 2013, and estimate the radio emission frequencies associated with these events. These stellar eruptions have proven to be elusive, although a promising approach to detect …

2022 The Astrophysical Journal
Gaia 12
Sh 2-301: A Blistered H II Region Undergoing Star Formation
DOI: 10.3847/1538-4357/ac41c3 Bibcode: 2022ApJ...926...25P

Pandey, Rakesh; Sharma, Saurabh; Panwar, Neelam +6 more

We present a multiwavelength study of the H II region Sh 2-301 (S301) using deep optical data, near-infrared data, radio continuum data, and other archival data at longer wavelengths. A cluster of young stellar objects (YSOs) is identified in the northeast (NE) direction of S301. The Hα and radio continuum images trace the distribution of the ioni…

2022 The Astrophysical Journal
AKARI Gaia 12
AT2020hur: A Possible Optical Counterpart of FRB 180916B
DOI: 10.3847/1538-4357/ac5d5a Bibcode: 2022ApJ...929..139L

Dai, Zi-Gao; Li, Long; Li, Qiao-Chu +4 more

The physical origin of fast radio bursts (FRBs) remains unclear. Finding multiwavelength counterparts of FRBs can provide a breakthrough for understanding their nature. In this work, we perform a systematic search for astronomical transients whose positions are consistent with FRBs. We find an unclassified optical transient AT2020hur (α = 01h…

2022 The Astrophysical Journal
INTEGRAL 12
Extreme Nature of Four Blue-excess Dust-obscured Galaxies Revealed by Optical Spectroscopy
DOI: 10.3847/1538-4357/aca403 Bibcode: 2022ApJ...941..195N

Ueda, Yoshihiro; Terashima, Yuichi; Matsuhara, Hideo +13 more

We report optical spectroscopic observations of four blue-excess dust-obscured galaxies (BluDOGs) identified by the Subaru Hyper Suprime-Cam. BluDOGs are a subclass of dust-obscured galaxies (DOGs; defined with the extremely red color (i - [22])AB ≥ 7.0; Toba et al., showing a significant flux excess in the optical g and r bands over th…

2022 The Astrophysical Journal
Herschel 12
The Proper Motion of the Pulsar J1124-5916 in the Galactic Supernova Remnant G292.0+1.8
DOI: 10.3847/1538-4357/ac704b Bibcode: 2022ApJ...932..117L

Long, Xi; Plucinsky, Paul P.; Patnaude, Daniel J. +1 more

We present the first direct measurement of the proper motion of pulsar J1124-5916 in the young, oxygen-rich supernova remnant G292.0+1.8. Using deep Chandra ACIS-I observations from 2006 to 2016, we measure a positional change of 0.″21 ± 0.″05 over the ~10 yr baseline, or ~0.″02 yr-1. At a distance of 6.2 ± 0.9 kpc, this corresponds to …

2022 The Astrophysical Journal
Gaia 12
The ESO-VLT MIKiS Survey Reloaded: Velocity Dispersion Profile and Rotation Curve of NGC 1904
DOI: 10.3847/1538-4357/ac5d4e Bibcode: 2022ApJ...929..186L

Vesperini, Enrico; Pallanca, Cristina; Dalessandro, Emanuele +8 more

We present an investigation of the internal kinematic properties of M79 (NGC 1904). Our study is based on radial velocity measurements obtained from the ESO-VLT Multi-Instrument Kinematic Survey (MIKiS) of Galactic globular clusters for more than 1700 individual stars distributed between ~0.″3 and 770″ (~14 three-dimensional half-mass radii) from …

2022 The Astrophysical Journal
Gaia eHST 12
Plasma Composition Measurements in an Active Region from Solar Orbiter/SPICE and Hinode/EIS
DOI: 10.3847/1538-4357/ac9b0b Bibcode: 2022ApJ...940...66B

Teriaca, Luca; Schmutz, Werner; Warren, Harry P. +28 more

A key goal of the Solar Orbiter mission is to connect elemental abundance measurements of the solar wind enveloping the spacecraft with extreme-UV (EUV) spectroscopic observations of their solar sources, but this is not an easy exercise. Observations from previous missions have revealed a highly complex picture of spatial and temporal variations o…

2022 The Astrophysical Journal
Hinode SolarOrbiter 12
Connecting Chromospheric Condensation Signatures to Reconnection-driven Heating Rates in an Observed Flare
DOI: 10.3847/1538-4357/ac402d Bibcode: 2022ApJ...926..164A

Qiu, Jiong; Longcope, Dana W.; Zhu, Chunming +1 more

Observations of solar flare reconnection at very high spatial and temporal resolution can be made indirectly at the footpoints of reconnected loops into which flare energy is deposited. The response of the lower atmosphere to this energy input includes a downward-propagating shock called chromospheric condensation, which can be observed in the UV …

2022 The Astrophysical Journal
IRIS 12