Search Publications

Galaxy Cluster Mass Estimates in the Presence of Substructure
DOI: 10.3847/1538-4357/ab609d Bibcode: 2020ApJ...888..106T

Mateo, Mario; Olszewski, Edward W.; Miller, Christopher J. +3 more

We develop and implement a model to analyze the internal kinematics of galaxy clusters that may contain subpopulations of galaxies that do not independently trace the cluster potential. The model allows for substructures within the cluster environment and disentangles cluster members from contaminating foreground and background galaxies. We estima…

2020 The Astrophysical Journal
XMM-Newton 4
Inferring Contributions from Unresolved Point Sources to Diffuse Emissions Measured in UV Sky Surveys: General Method and SOHO/SWAN Case Study
DOI: 10.3847/1538-4357/ab9e6f Bibcode: 2020ApJ...899...48S

Bzowski, M.; Kubiak, M. A.; Kowalska-Leszczynska, I. +1 more

In observations of diffuse emissions like, e.g., the Lyα heliospheric glow, contributions to the observed signal from point sources (e.g., stars) are considered to be a contamination. There are relatively few bright point sources that are usually properly resolved and can be subtracted or masked. We present results of an analysis of the distributi…

2020 The Astrophysical Journal
IUE SOHO 4
Termination Shock as a Source of Unusual Solar Radio Bursts
DOI: 10.3847/1538-4357/abad9f Bibcode: 2020ApJ...901...65F

Chernov, Gennady; Fomichev, Valery

Using centimeter-wave and decimeter-wave solar radio spectral observations of the flares of 2003 November 18 and 2004 September 12, we have discussed two type-II-like bursts at the meter waves. The radio bursts show that the ordinary frequency drift from high to low frequencies slows down and stops, and a frequency drift from low to high frequenci…

2020 The Astrophysical Journal
SOHO 4
The Energetic Thermonuclear Bursts in SAX J1712.6-3739
DOI: 10.3847/1538-4357/abb76f Bibcode: 2020ApJ...903...37L

Lin, Jie; Yu, Wenfei

The neutron star low-mass X-ray binary SAX J1712.6-3739 is known for its long and hard thermonuclear X-ray bursts from previous observations. Its thermonuclear bursts are so distinct as they can last for tens of minutes, as seen with Swift/BAT (E > 15 keV). To explore the origin of these extreme bursts and the nature of SAX J1712.6-3739, we ana…

2020 The Astrophysical Journal
INTEGRAL 4
The Dynamics of the Magnetic-field-free Cavity around Comets
DOI: 10.3847/1538-4357/ab6e69 Bibcode: 2020ApJ...891..112N

Nemeth, Z.

The diamagnetic cavity is the innermost region of the magnetosphere of an active comet, from which the magnetic field is expelled by the outflowing matter. This phenomenon, first detected around comet 1P/Halley, was extensively studied recently by the Rosetta comet chaser mission. Rosetta observed a surprisingly large diamagnetic cavity around com…

2020 The Astrophysical Journal
Rosetta 4
Localized Amplification of Magnetic Field in the Solar Photosphere Associated with a Rapid Moving Pore
DOI: 10.3847/2041-8213/abb096 Bibcode: 2020ApJ...900L..17X

Yang, Bo; Yang, Jiayan; Bi, Yi +4 more

In the Sun, the flows of hot plasma drive a dynamo that generates a global magnetic field as well as smaller-scale local fields. The existence of a magnetic field in turn affects the motion of plasma so that complex dynamic characteristics can be observed. In this Letter, we give an analysis on the localized amplification of magnetic fields in fro…

2020 The Astrophysical Journal
IRIS 3
A Large Massive Quiescent Galaxy Sample at z ∼ 1.2
DOI: 10.3847/1538-4357/abbeff Bibcode: 2020ApJ...905..103X

Sawicki, Marcin; Cheng, Cheng; Huang, Jia-Sheng +8 more

In this paper we present a simple color-magnitude selection and obtain a large sample of 33,893 massive quiescent galaxies at intermediate redshifts (1 < z < 1.5). We choose the longest wavelength available in the Hyper-Supreme-Cam (HSC) deep survey, the Y band and i - Y color, to select the 4000 Å Balmer jump in passive galaxies to the high…

2020 The Astrophysical Journal
eHST 3
Variability of the Great Disk Shadow in Serpens
DOI: 10.3847/1538-4357/ab91ae Bibcode: 2020ApJ...896..169P

Green, Joel D.; Pontoppidan, Klaus M.; Salyk, Colette +2 more

We present dual-epoch Hubble Space Telescope imaging of the great disk shadow in the Serpens star-forming region. The near-infrared images show strong variability of the disk shadow, revealing dynamics of the inner disk on timescales of months. The Great Shadow is projected onto the Serpens reflection nebula by an unresolved protoplanetary disk su…

2020 The Astrophysical Journal
Herschel eHST 3
A Detailed Analysis of the Cloud Structure and Dynamics in Aquila Rift
DOI: 10.3847/1538-4357/ab8c4f Bibcode: 2020ApJ...895..137S

Nakamura, Fumitaka; Dobashi, Kazuhito; Shimoikura, Tomomi +1 more

We present maps in several molecular emission lines of a 1 square degree region covering the W40 and Serpens South molecular clouds belonging to the Aquila Rift complex. The observations were made with the 45 m telescope at the Nobeyama Radio Observatory. We found that the 12CO and 13CO emission lines consist of several veloc…

2020 The Astrophysical Journal
Herschel 3
Softening of the Metagalactic Ionizing Background from Internal He II Absorption in Quasars
DOI: 10.3847/1538-4357/aba3c9 Bibcode: 2020ApJ...899..163S

Shull, J. Michael; Danforth, Charles W.

Quasars and other active galactic nuclei (AGN) are significant contributors to the metagalactic ionizing background at redshifts z < 3. Recent Hubble Space Telescope (HST)/Cosmic Origins Spectrograph (COS) composite spectra of AGN find a harder flux distribution in the Lyman continuum, ${F}_{\nu }\propto {\nu }^{-{\alpha }_{s}}$ (αs

2020 The Astrophysical Journal
eHST 3