Search Publications

An Optical Spectrum of the Diffuse Galactic Light from BOSS and IRIS
DOI: 10.3847/1538-4357/ac6efc Bibcode: 2022ApJ...932..112C

Hensley, Brandon S.; Brandt, Timothy D.; Draine, Bruce T. +2 more

We present a spectrum of the diffuse Galactic light (DGL) between 3700 and 10,000 Å, obtained by correlating optical sky intensity with far-infrared dust emission. We use nearly 250,000 blank-sky spectra from BOSS/SDSS-III together with IRIS-reprocessed maps from the IRAS satellite. The larger sample size compared to SDSS-II results in a factor-of…

2022 The Astrophysical Journal
Gaia 7
A White Dwarf-Main-sequence Binary Unveiled by Time-domain Observations from LAMOST and TESS
DOI: 10.3847/1538-4357/ac853f Bibcode: 2022ApJ...936...33Z

Liu, Jifeng; Zong, Weikai; Bai, Yu +16 more

We report a single-lined white dwarf-main-sequence binary system, LAMOST J172900.17+652952.8, which is discovered by the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST)'s medium-resolution time-domain surveys. The radial-velocity semi-amplitude and orbital period of the optical visible star are measured by using follow-up observ…

2022 The Astrophysical Journal
Gaia 7
Validation and Interpretation of a Three-dimensional Configuration of a Magnetic Cloud Flux Rope
DOI: 10.3847/1538-4357/ac7803 Bibcode: 2022ApJ...934...50H

Qiu, Jiong; Hu, Qiang; Jian, Lan K. +3 more

One strong magnetic cloud (MC) with a magnetic field magnitude reaching ~40 nT at 1 au during 2012 June 16-17 is examined in association with a preexisting magnetic flux rope (MFR) identified on the Sun. The MC is characterized by a quasi-three-dimensional (3D) flux rope model based on in situ measurements from the Wind spacecraft. The contents of…

2022 The Astrophysical Journal
SOHO VenusExpress 7
Further Evidence for the Minifilament-eruption Scenario for Solar Polar Coronal Jets
DOI: 10.3847/1538-4357/ac473e Bibcode: 2022ApJ...927...79B

Savcheva, Antonia; Moore, Ronald L.; Savage, Sabrina L. +4 more

We examine a sampling of 23 polar-coronal-hole jets. We first identified the jets in soft X-ray (SXR) images from the X-ray telescope (XRT) on the Hinode spacecraft, over 2014-2016. During this period, frequently the polar holes were small or largely obscured by foreground coronal haze, often making jets difficult to see. We selected 23 jets among…

2022 The Astrophysical Journal
Hinode 7
A Morphological Study of Galaxies Hosting Optical Variability-selected AGNs in the COSMOS Field
DOI: 10.3847/1538-4357/ac3edb Bibcode: 2022ApJ...925..157Z

Inoue, Akio K.; Yamada, Toru; Zhong, Yuxing +1 more

Morphological studies are crucial to investigate the connections between active galactic nucleus (AGN) activities and the evolution of galaxies. Substantial studies have found that radiative-mode AGNs primarily reside in disk galaxies, questioning the merger-driven mechanism of AGN activities. In this study, through Sérsic profile fitting and nonp…

2022 The Astrophysical Journal
AKARI eHST 7
Testing the Potential for Radio Variability in Disks around T Tauri Stars with Observations and Chemical Modeling
DOI: 10.3847/1538-4357/ac365a Bibcode: 2022ApJ...924..104E

Calvet, N.; D'Alessio, P.; Macías, E. +5 more

A multiwavelength observing campaign of the T Tauri star (TTS) GM Aur was undertaken in 2019 December. This campaign obtained Swift X-ray and NUV fluxes, HST NUV spectra, LCOGT ${u}^{{\prime} }> ${g}^{{\prime} }> ${r}^{{\prime} }> ${i}^{{\prime} }> and TESS photometry, CHIRON Hα spectra, Atacama Large Millimeter/submillimeter Array (AL…

2022 The Astrophysical Journal
eHST 7
Topography of the Young Galactic Disk: Spatial and Kinematic Patterns of Clustered Star Formation in the Solar Neighborhood
DOI: 10.3847/1538-4357/ac8b0c Bibcode: 2022ApJ...937..114A

González, Marta; Alfaro, Emilio J.; Sánchez-Gil, M. Carmen +3 more

The accuracy in determining the spatial-kinematical parameters of open clusters makes them ideal tracers of the Galactic structure. Young open clusters (YOCs) are the main representatives of the clustered star formation mode, which identifies how most of the stars in the Galaxy form. We apply the Kriging technique to a sample of Gaia YOCs within a…

2022 The Astrophysical Journal
Gaia 7
Dissecting the Extended X-Ray Emission in the Merging Pair NGC 6240: Photoionization and Winds
DOI: 10.3847/1538-4357/ac5025 Bibcode: 2022ApJ...927..166P

Elvis, M.; Fabbiano, G.; Nardini, E. +3 more

We present a detailed spectral and imaging analysis of the central 15″ radius (~7.5 kpc) region of the merger galaxy NGC 6240 that makes use of all the available Chandra-ACIS data (0.3-3 keV effective exposure of ~190 ks). This region shows extended X-ray structures with lower-energy counterparts imaged in CO, [O III], and Hα line emission. We fin…

2022 The Astrophysical Journal
eHST 7
1RXH J082623.6-505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate
DOI: 10.3847/1538-4357/ac7b25 Bibcode: 2022ApJ...934..142S

Strader, Jay; Bahramian, Arash; Chomiuk, Laura +13 more

We report the discovery of 1RXH J082623.6-505741, a 10.4 hr orbital period compact binary. Modeling extensive optical photometry and spectroscopy reveals a ~0.4 M K-type secondary transferring mass through a low-state accretion disk to a nonmagnetic ~0.8 M white dwarf. The secondary is overluminous for its mass and domina…

2022 The Astrophysical Journal
Gaia XMM-Newton 7
The Host Galaxy of the Recoiling Black Hole Candidate in 3C 186: An Old Major Merger Remnant at the Center of a z = 1 Cluster
DOI: 10.3847/1538-4357/ac6a58 Bibcode: 2022ApJ...931..165M

Bianchi, S.; Macchetto, F. D.; Capetti, A. +10 more

3C 186, a radio-loud quasar at z = 1.0685, was previously reported to have both velocity and spatial offsets from its host galaxy, and has been considered as a promising candidate for a gravitational wave recoiling black hole triggered by a black hole merger. Another possible scenario is that 3C 186 is in an ongoing galaxy merger, exhibiting a tem…

2022 The Astrophysical Journal
eHST 7