Search Publications

Hot Gas in Galaxy Halos Traced by Coronal Broad Lyα Absorbers
DOI: 10.3847/1538-4357/ab7937 Bibcode: 2020ApJ...892...33R

Richter, Philipp

We explore the possibility to systematically study the extended, hot gaseous halos of low-redshift galaxies with coronal broad Lyα absorbers (CBLAs). These are weak, thermally broadenend H I absorption lines arising from the tiny fraction of neutral hydrogen that resides in the collisionally ionized, million-degree halo gas in these galaxies. Usin…

2020 The Astrophysical Journal
eHST 5
A Catalog of 531 White Dwarf Candidates in the Local Galactic Halo from Gaia Data Release 2
DOI: 10.3847/1538-4357/aba523 Bibcode: 2020ApJ...899...83K

Kim, Bokyoung; Lépine, Sebastien; Medan, Ilija

We present a catalog of 531 white dwarf candidates that have large apparent transverse motions relative to the Sun ( ${v}_{T}\gt 200$ km s-1), thus making them likely members of the local Galactic halo population. The candidates were selected from the Gaia Data Release 2 and are located in a great circle with 20° width running across bo…

2020 The Astrophysical Journal
Gaia 5
KIC 12268220: A δ Scuti Pulsating Star and an Active Protohelium White Dwarf in an Eclipsing Binary System
DOI: 10.3847/1538-4357/ab9b85 Bibcode: 2020ApJ...898..136C

Liu, Jifeng; Gao, Qing; Ren, Juanjuan +4 more

We present a photometric, spectroscopic, asteroseismic, and evolutionary analysis of the Algol-type eclipsing binary KIC 12268220. We find the O'Connell effect and anticorrelated eclipse timing variations in the Kepler light curve, revealing the presence of large starspots. Radial velocities and atmospheric parameters are obtained from ground-base…

2020 The Astrophysical Journal
Gaia 5
NuSTAR Observations and Multiwavelength Modeling of the High-redshift BL Lacertae Object 4FGL J2146.5-1344
DOI: 10.3847/1538-4357/ab6226 Bibcode: 2020ApJ...889..102R

Ajello, M.; Kaur, A.; Hartmann, D. +3 more

High synchrotron peak (HSP; ${\nu }_{\mathrm{sy}}^{\mathrm{pk}}\gt {10}^{15}$ Hz) BL Lac objects are some of the most extreme accelerators in the universe. Those found at high redshifts (z > 1) challenge our understanding of blazar evolution models and are crucial for cosmological measurements of the extragalactic background light. In this pape…

2020 The Astrophysical Journal
XMM-Newton 5
A Strong-lensing Model for the WMDF JWST/GTO Very Rich Cluster A1489
DOI: 10.3847/1538-4357/abb8dd Bibcode: 2020ApJ...903..137Z

Finkelstein, Steven L.; Koekemoer, Anton M.; Larson, Rebecca L. +19 more

We present a first strong-lensing model for the galaxy cluster RM J121218.5+273255.1 (z = 0.35; hereafter RMJ1212; also known as A1489). This cluster is among the top 0.1% richest clusters in the redMaPPer catalog; it is significantly detected in X-ray and through the Sunyaev-Zel'dovich effect in ROSAT and Planck data, respectively, and its optica…

2020 The Astrophysical Journal
eHST 5
Dynamical Masses for the Pleiades Binary System HII-2147
DOI: 10.3847/1538-4357/ab9c20 Bibcode: 2020ApJ...898....2T

Torres, Guillermo; Crepp, Justin R.; Dupuy, Trent J. +3 more

We report our long-term spectroscopic monitoring of the Pleiades member HII-2147, which was previously spatially resolved at radio wavelengths in very long baseline interferometry (VLBI) observations. It has also been claimed to be a (presumably short-period) double-lined spectroscopic binary with relatively sharp lines, although no orbit has ever…

2020 The Astrophysical Journal
Gaia 5
Unraveling the Nature of the Deeply Embedded Wolf-Rayet Star WR 121a
DOI: 10.3847/1538-4357/ab7337 Bibcode: 2020ApJ...891..104A

Pandey, J. C.; Arora, Bharti

An X-ray study of the deeply embedded Wolf-Rayet star WR 121a has been carried out using long-term (spanning over ∼12 yr) archival observations from Chandra and XMM-Newton. For the first time, a periodic variation of 4.1 days has been detected in the X-ray light curve of WR 121a. No companion is seen in a merged and exposure-corrected Chandra X-ra…

2020 The Astrophysical Journal
XMM-Newton 5
Fast Magnetosonic Waves and Flows in a Solar Prominence Foot: Observations and Modeling
DOI: 10.3847/1538-4357/aba2eb Bibcode: 2020ApJ...899...99O

Ofman, Leon; Kucera, Therese A.

We study recent observations of propagating fluctuations in a prominence foot with Hinode Solar Optical Telescope (SOT) high-resolution observations in Ca II and Hα emission, which we identify as nonlinear fast magnetosonic waves. Here we analyze further the observations of propagating waves and flows with Interface Region Imaging Spectrograph Mg …

2020 The Astrophysical Journal
Hinode IRIS 5
A New Metal-poor Globular Cluster and Resolved Stars in the Outer Disk of the Black Eye Galaxy M64: Implication for the Origin of the Type III Disk Break
DOI: 10.3847/1538-4357/ab94ba Bibcode: 2020ApJ...897..106K

Lee, Myung Gyoon; Kang, Jisu; Jang, In Sung +1 more

M64 is a nearby spiral galaxy with a Type III antitruncation component. To trace the origin of the Type III component, we present Hubble Space Telescope/Advanced Camera for Surveys (ACS) F606W/F814W photometry of resolved stars in a field located in the outer disk ( $2\buildrel{\,\prime}\over{.} 5\lesssim r\lesssim 6\buildrel{\,\prime}\over{.} 5$ …

2020 The Astrophysical Journal
eHST 5
NuSTAR Observations of G11.2-0.3
DOI: 10.3847/1538-4357/ab54ca Bibcode: 2020ApJ...889...23M

Fryer, C. L.; Grefenstette, B. W.; Madsen, K. K. +3 more

We present in this paper the hard X-ray view of the pulsar wind nebula in G11.2-0.3 and its central pulsar powered pulsar J1811-1925 as seen by NuSTAR. We complement the data with Chandra for a more complete picture and confirm the existence of a hard, power-law component in the shell with photon index ${\rm{\Gamma }}=2.1\pm 0.1$ , which we attrib…

2020 The Astrophysical Journal
INTEGRAL 5