Search Publications

A Hard Look at Local, Optically Selected, Obscured Seyfert Galaxies
DOI: 10.3847/1538-4357/abb29f Bibcode: 2020ApJ...901..161K

Kaastra, J. S.; Stern, D.; Brandt, W. N. +11 more

We study the X-ray spectra of a sample of 19 obscured, optically selected Seyfert galaxies (Sy 1.8, 1.9, and 2) in the local universe (d ≤ 175 Mpc), drawn from the CfA Seyfert sample. Our analysis is driven by the high sensitivity of NuSTAR in the hard X-rays, coupled with soft X-ray spectra using XMM-Newton, Chandra, Suzaku, and Swift/XRT. We als…

2020 The Astrophysical Journal
Suzaku XMM-Newton 23
Direct Measurement of the Solar-wind Taylor Microscale Using MMS Turbulence Campaign Data
DOI: 10.3847/1538-4357/ab9ebe Bibcode: 2020ApJ...899...63B

Strangeway, Robert J.; Russell, Christopher T.; Chasapis, Alexandros +7 more

Using the novel Magnetospheric Multiscale (MMS) mission data accumulated during the 2019 MMS Solar Wind Turbulence Campaign, we calculate the Taylor microscale (λT) of the turbulent magnetic field in the solar wind. The Taylor microscale represents the onset of dissipative processes in classical turbulence theory. However, an accurate e…

2020 The Astrophysical Journal
Cluster 23
Diagonal Ridge Pattern of Different Age Populations Found in Gaia-DR2 with LAMOST Main-sequence Turnoff and OB-type Stars
DOI: 10.3847/1538-4357/abb3c8 Bibcode: 2020ApJ...902...70W

Wang, H. -F.; López-Corredoira, M.; Huang, Y. +5 more

We revisit the diagonal ridge feature (diagonal distributions in the R, vφ plane) found in Gaia and present a timing analysis for it between Galactocentric distances of R = 7.5 and 12 kpc, using main-sequence turnoff and OB stars selected from the LAMOST Galactic spectroscopic surveys. We recover the ridge pattern in the R-vφ

2020 The Astrophysical Journal
Gaia 23
Dependence of the IRX-β Dust Attenuation Relation on Metallicity and Environment
DOI: 10.3847/2041-8213/abc1ef Bibcode: 2020ApJ...903L..28S

Shivaei, Irene; Mobasher, Bahram; Scoville, Nick +4 more

We use a sample of star-forming field and protocluster galaxies at z = 2.0-2.5 with Keck/MOSFIRE K-band spectra, a wealth of rest-frame ultraviolet (UV) photometry, and Spitzer/MIPS and Herschel/PACS observations, to dissect the relation between the ratio of infrared (IR) to UV luminosity (IRX) versus UV slope (β) as a function of gas-phase metall…

2020 The Astrophysical Journal
Herschel 23
A Massive Molecular Torus inside a Gas-poor Circumnuclear Disk in the Radio Galaxy NGC 1052 Discovered with ALMA
DOI: 10.3847/1538-4357/ab8bd6 Bibcode: 2020ApJ...895...73K

Kohno, Kotaro; Terashima, Yuichi; Nakai, Naomasa +7 more

We report ALMA observations of NGC 1052 to search for mass accretion in a gas-poor active galactic nucleus. We detected CO emission representing a rotating ring-like circumnuclear disk (CND) seen edge-on with a gas mass of 5.3 × 105 M. The CND has smaller gas mass than that in typical Seyfert galaxies with circumnuclear star…

2020 The Astrophysical Journal
eHST 23
TOI-1728b: The Habitable-zone Planet Finder Confirms a Warm Super-Neptune Orbiting an M-dwarf Host
DOI: 10.3847/1538-4357/aba0a2 Bibcode: 2020ApJ...899...29K

Cochran, William D.; Endl, Michael; Mahadevan, Suvrath +23 more

We confirm the planetary nature of TOI-1728b using a combination of ground-based photometry, near-infrared Doppler velocimetry and spectroscopy with the Habitable-zone Planet Finder. TOI-1728 is an old, inactive M0 star with Teff = ${3980}_{-32}^{+31}$ K, which hosts a transiting super-Neptune at an orbital period of ∼3.49 days. Joint f…

2020 The Astrophysical Journal
Gaia 23
HD 62542: Probing the Bare, Dense Core of a Translucent Interstellar Cloud
DOI: 10.3847/1538-4357/ab8f8e Bibcode: 2020ApJ...897...36W

York, Donald G.; Welty, Daniel E.; Snow, Theodore P. +1 more

We discuss the interstellar absorption from many atomic and molecular species seen in high-resolution Hubble Space Telescope/STIS UV and high signal-to-noise ratio optical spectra of the moderately reddened B3-5 V star HD 62542. This remarkable sight line exhibits both very steep far-UV extinction and a high fraction of hydrogen in molecular form,…

2020 The Astrophysical Journal
eHST 23
Is Extended Hard X-Ray Emission Ubiquitous in Compton-thick AGN?
DOI: 10.3847/1538-4357/abacbe Bibcode: 2020ApJ...900..164M

Elvis, Martin; Risaliti, Guido; Fabbiano, G. +4 more

The recent Chandra discovery of extended ∼kiloparsec-scale hard (>3 keV) X-ray emission in nearby Compton-thick (CT) active galactic nuclei (AGN) opens a new window to improving AGN torus modeling and investigating how the central supermassive black hole interacts with and impacts the host galaxy. Since there are only a handful of detections so…

2020 The Astrophysical Journal
eHST 23
Inverse First Ionization Potential Effects in Giant Solar Flares Found from Earth X-Ray Albedo with Suzaku/XIS
DOI: 10.3847/1538-4357/ab7207 Bibcode: 2020ApJ...891..126K

Maeda, Yoshitomo; Katsuda, Satoru; Sato, Kosuke +21 more

We report X-ray spectroscopic results for four giant solar flares that occurred on 2005 September 7 (X17.0), 2005 September 8 (X5.4), 2005 September 9 (X6.2), and 2006 December 5 (X9.0), obtained from Earth albedo data with the X-ray Imaging Spectrometer (XIS) on board Suzaku. The good energy resolution of the XIS (FWHM ∼ 100 eV) enables us to sep…

2020 The Astrophysical Journal
Suzaku 23
Magnetosheath Jets and Plasmoids: Characteristics and Formation Mechanisms from Hybrid Simulations
DOI: 10.3847/2041-8213/abad2b Bibcode: 2020ApJ...900L...6P

Blanco-Cano, Xóchitl; Burgess, David; Trotta, Domenico +2 more

Magnetosheath jets and plasmoids are very common phenomena downstream of Earth's quasi-parallel bow shock. As the increase of the dynamic pressure is one of the principal characteristics of magnetosheath jets, the embedded paramagnetic plasmoids have been considered as an special case of the former. Although the properties of both types of structu…

2020 The Astrophysical Journal
Cluster 23