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Simultaneous Chandra and VLA Observations of the Transitional Millisecond Pulsar PSR J1023+0038: Anti-correlated X-Ray and Radio Variability
DOI: 10.3847/1538-4357/aaaeb9 Bibcode: 2018ApJ...856...54B

Deller, Adam T.; Bogdanov, Slavko; Hessels, Jason W. T. +6 more

We present coordinated Chandra X-ray Observatory and Karl G. Jansky Very Large Array observations of the transitional millisecond pulsar PSR J1023+0038 in its low-luminosity accreting state. The unprecedented five hours of strictly simultaneous X-ray and radio continuum coverage for the first time unambiguously show a highly reproducible, anti-cor…

2018 The Astrophysical Journal
XMM-Newton 59
Revealing the Environmental Dependence of Molecular Gas Content in a Distant X-Ray Cluster at z = 2.51
DOI: 10.3847/2041-8213/aaeb2c Bibcode: 2018ApJ...867L..29W

Kohno, Kotaro; Daddi, Emanuele; Koyama, Yusei +13 more

We present a census of the molecular gas properties of galaxies in the most distant known X-ray cluster, CLJ1001, at z = 2.51, using deep observations of CO(1-0) with the Karl G. Jansky Very Large Array. In total, 14 cluster members with M * > 1010.5 M are detected, including all of the massive star-forming me…

2018 The Astrophysical Journal
eHST 58
A New Relativistic Component of the Accretion Disk Wind in PDS 456
DOI: 10.3847/2041-8213/aaaae1 Bibcode: 2018ApJ...854L...8R

Reeves, J. N.; Braito, V.; Nardini, E. +3 more

Past X-ray observations of the nearby luminous quasar PDS 456 (at z = 0.184) have revealed a wide angle accretion disk wind, with an outflow velocity of ∼-0.25c. Here, we unveil a new, relativistic component of the wind through hard X-ray observations with NuSTAR and XMM-Newton, obtained in 2017 March when the quasar was in a low-flux state. This …

2018 The Astrophysical Journal
XMM-Newton 58
A Long Decay of X-Ray Flux and Spectral Evolution in the Supersoft Active Galactic Nucleus GSN 069
DOI: 10.3847/2041-8213/aaba17 Bibcode: 2018ApJ...857L..16S

Shu, X. W.; Wang, J. X.; Wang, T. G. +3 more

GSN 069 is an optically identified very low-mass active galactic nuclei (AGN) that shows supersoft X-ray emission. The source is known to exhibit a huge X-ray outburst, with flux increased by more than a factor of ∼240 compared to the quiescence state. We report its long-term evolution in the X-ray flux and spectral variations over a timescale of …

2018 The Astrophysical Journal
XMM-Newton 58
Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. II. Spatially Resolved Mass Outflow Rates for the QSO2 Markarian 34
DOI: 10.3847/1538-4357/aae3e6 Bibcode: 2018ApJ...867...88R

Kraemer, S. B.; Crenshaw, D. M.; Gandhi, P. +10 more

We present spatially resolved mass outflow rate measurements ({\dot{M}}out}) for the narrow line region of Markarian 34, the nearest Compton-thick type 2 quasar (QSO2). Spectra obtained with the Hubble Space Telescope and at Apache Point Observatory reveal complex kinematics, with distinct signatures of outflow and rotation within 2 kpc…

2018 The Astrophysical Journal
eHST 58
Molecular Gas Contents and Scaling Relations for Massive, Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey
DOI: 10.3847/1538-4357/aac438 Bibcode: 2018ApJ...860..103S

Muzzin, Adam; van Dokkum, Pieter; van der Wel, Arjen +13 more

A decade of study has established that the molecular gas properties of star-forming galaxies follow coherent scaling relations out to z ∼ 3, suggesting remarkable regularity of the interplay between molecular gas, star formation, and stellar growth. Passive galaxies, however, are expected to be gas-poor and therefore faint, and thus little is know…

2018 The Astrophysical Journal
eHST 58
Dual Phase-space Cascades in 3D Hybrid-Vlasov-Maxwell Turbulence
DOI: 10.3847/2041-8213/aab557 Bibcode: 2018ApJ...856L..13C

Califano, F.; Cerri, S. S.; Kunz, M. W.

To explain energy dissipation via turbulence in collisionless, magnetized plasmas, the existence of a dual real- and velocity-space cascade of ion-entropy fluctuations below the ion gyroradius has been proposed. Such a dual cascade, predicted by the gyrokinetic theory, has previously been observed in gyrokinetic simulations of two-dimensional, ele…

2018 The Astrophysical Journal
Cluster 58
Unveiling the Dynamical State of Massive Clusters through the ICL Fraction
DOI: 10.3847/1538-4357/aab70f Bibcode: 2018ApJ...857...79J

Koekemoer, Anton M.; Donahue, Megan; Frye, Brenda L. +34 more

We have selected a sample of 11 massive clusters of galaxies observed by the Hubble Space Telescope in order to study the impact of the dynamical state on the intracluster light (ICL) fraction, the ratio of total integrated ICL to the total galaxy member light. With the exception of the Bullet cluster, the sample is drawn from the Cluster Lensing …

2018 The Astrophysical Journal
eHST 57
Ionized and Molecular Gas Kinematics in a z = 1.4 Star-forming Galaxy
DOI: 10.3847/2041-8213/aaacfa Bibcode: 2018ApJ...854L..24U

Lutz, D.; Wuyts, S.; Förster Schreiber, N. M. +17 more

We present deep observations of a z = 1.4 massive, star-forming galaxy (SFG) in molecular and ionized gas at comparable spatial resolution (CO 3-2, NOrthern Extended Millimeter Array (NOEMA); Hα, Large Binocular Telescope (LBT)). The kinematic tracers agree well, indicating that both gas phases are subject to the same gravitational potential and p…

2018 The Astrophysical Journal
eHST 57
The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
DOI: 10.3847/1538-4357/aac3d9 Bibcode: 2018ApJ...860..104U

Donahue, Megan; Broadhurst, Tom; Zitrin, Adi +24 more

We reconstruct the two-dimensional (2D) matter distributions in 20 high-mass galaxy clusters selected from the CLASH survey by using the new approach of performing a joint weak gravitational lensing analysis of 2D shear and azimuthally averaged magnification measurements. This combination allows for a complete analysis of the field, effectively br…

2018 The Astrophysical Journal
eHST 57