Search Publications

A Joint NICER and XMM-Newton View of the “Magnificent” Thermally Emitting X-Ray Isolated Neutron Star RX J1605.3+3249
DOI: 10.3847/1538-4357/ab2875 Bibcode: 2019ApJ...880...74M

Enoto, Teruaki; Bogdanov, Slavko; Ray, Paul S. +11 more

Thermally emitting X-ray isolated neutron stars (NSs) represent excellent targets for testing cooling surface emission and atmosphere models, which are used to infer the physical parameters of the NS. Among the seven known members of this class, RX J1605.3+3249 is the only one that still lacks confirmation of its spin period. Here we analyze NICER…

2019 The Astrophysical Journal
XMM-Newton 14
Solar Active Region Heating Diagnostics from High-temperature Emission Using the MaGIXS
DOI: 10.3847/1538-4357/ab3eb4 Bibcode: 2019ApJ...884...24A

Golub, Leon; Winebarger, Amy R.; Warren, Harry P. +7 more

The relative amount of high-temperature plasma has been found to be a useful diagnostic to determine the frequency of coronal heating on sub-resolution structures. When the loops are infrequently heated, a broad emission measure (EM) over a wider range of temperatures is expected. A narrower EM is expected for high-frequency heating where the loop…

2019 The Astrophysical Journal
Hinode 14
Monitoring the Superorbital Period Variation and Spin Period Evolution of SMC X-1
DOI: 10.3847/1538-4357/ab48e4 Bibcode: 2019ApJ...885..123H

Enoto, Teruaki; Ueda, Yoshihiro; Hu, Chin-Ping +2 more

The X-ray pulsar SMC X-1 shows a superorbital modulation with an unstable cycle length in the X-ray band. We present its timing behaviors, including the spin, orbital, and superorbital modulations, beyond the end of the Rossi X-ray Timing Explorer mission. The time-frequency maps derived by the wavelet Z-transform and the Hilbert-Huang transform s…

2019 The Astrophysical Journal
XMM-Newton 14
Hubble Space Telescope Spectroscopy of a Planetary Nebula in an M31 Open Cluster: Hot-bottom Burning at 3.4 M
DOI: 10.3847/1538-4357/ab44d4 Bibcode: 2019ApJ...884..115D

Bond, Howard E.; Ciardullo, Robin; Jacoby, George H. +1 more

We use imaging and spectroscopy from the Hubble Space Telescope (HST) to examine the properties of a bright planetary nebula (PN) projected within M31's young open cluster B477-D075. We show that the probability of a chance superposition of the PN on the cluster is small, ≲2%. Moreover, the radial velocity of the PN is the same as that of the clus…

2019 The Astrophysical Journal
Gaia eHST 14
The Atacama Cosmology Telescope: CO(J = 3 - 2) Mapping and Lens Modeling of an ACT-selected Dusty Star-forming Galaxy
DOI: 10.3847/1538-4357/ab264b Bibcode: 2019ApJ...879...95R

Gallardo, Patricio A.; Huffenberger, Kevin M.; Hughes, John P. +13 more

We report Northern Extended Millimeter Array CO(J = 3 - 2) observations of the dusty star-forming galaxy ACT-S J020941+001557 at z = 2.5528, which was detected as an unresolved source in the Atacama Cosmology Telescope (ACT) equatorial survey. Our spatially resolved spectral line data support the derivation of a gravitational lens model from 37 in…

2019 The Astrophysical Journal
eHST 14
Benchmarking Substellar Evolutionary Models Using New Age Estimates for HD 4747 B and HD 19467 B
DOI: 10.3847/1538-4357/aafe01 Bibcode: 2019ApJ...873...83W

Crepp, Justin R.; White, Timothy R.; Brewer, John M. +5 more

Constraining substellar evolutionary models (SSEMs) is particularly difficult due to a degeneracy between the mass, age, and luminosity of a brown dwarf. In cases where a brown dwarf is found as a directly imaged companion to a star, as in HD 4747 and HD 19467, the mass, age, and luminosity of the brown dwarf are determined independently, making t…

2019 The Astrophysical Journal
Gaia 14
A Wide-field Photometric Survey of Globular Clusters in the Peculiar Early-type Galaxy M85
DOI: 10.3847/1538-4357/ab0306 Bibcode: 2019ApJ...872..202K

Park, Byeong-Gon; Hwang, Narae; Lee, Myung Gyoon +4 more

We survey globular clusters (GCs) in M85 using ugi-band images of a 1° × 1° field obtained with the MegaCam at the 3.6 m Canada-France-Hawaii Telescope. We identify 1318 GC candidates with 20.0 mag < g 0 < 23.5 mag in the entire survey region. Their radial number density profile is well fit by a Sérsic profile with n = {2.58}

2019 The Astrophysical Journal
eHST 14
Multifractal Analysis of Heliospheric Magnetic Field Fluctuations Observed by Ulysses
DOI: 10.3847/1538-4357/ab1750 Bibcode: 2019ApJ...876..153W

Bruno, Roberto; Wawrzaszek, Anna; Echim, Marius

We present the multifractal study of the intermittency of the magnetic field turbulence in the fast and slow solar wind beyond the ecliptic plane during two solar minima (1997-1998, 2007-2008) and solar maximum (1999-2001). More precisely, we consider 126 time intervals of Ulysses magnetic field measurements, obtain the multifractal spectra, and e…

2019 The Astrophysical Journal
Ulysses 14
Late-time Observations of the Type Ia Supernova SN 2014J with the Hubble Space Telescope Wide Field Camera 3
DOI: 10.3847/1538-4357/aaf1c3 Bibcode: 2019ApJ...870...14G

Graur, Or

Recent works have studied the late-time light curves of Type Ia supernovae (SNe Ia) when these were older than 500 days past B-band maximum light. Of these, SN 2014J, which exploded in the nearby galaxy M82, was studied with the Advanced Camera for Surveys onboard the Hubble Space Telescope (HST) by Yang et al. Here, I report complementary photome…

2019 The Astrophysical Journal
eHST 14
A Dynamical Study of Extraplanar Diffuse Ionized Gas in NGC 5775
DOI: 10.3847/1538-4357/ab4904 Bibcode: 2019ApJ...885..160B

Gallagher, J. S., III; Boettcher, Erin; Zweibel, Ellen G.

The structure and kinematics of gaseous, disk-halo interfaces are imprinted with the processes that transfer mass, metals, and energy between galactic disks and their environments. We study the extraplanar diffuse ionized gas (eDIG) layer in the interacting, star-forming galaxy NGC 5775 to better understand the consequences of star formation feedb…

2019 The Astrophysical Journal
eHST 14