Search Publications

Gemini Near Infrared Field Spectrograph Observations of the Seyfert 2 Galaxy Mrk 573: In Situ Acceleration of Ionized and Molecular Gas off Fueling Flows
DOI: 10.3847/1538-4357/834/1/30 Bibcode: 2017ApJ...834...30F

Kraemer, S. B.; Crenshaw, D. M.; Storchi-Bergmann, T. +9 more

We present near-infrared and optical emission-line and stellar kinematics of the Seyfert 2 galaxy Mrk 573 using the Near-Infrared Field Spectrograph (NIFS) at Gemini North and Dual Imaging Spectrograph at Apache Point Observatory, respectively. By obtaining full kinematic maps of the infrared ionized and molecular gas and stellar kinematics in a ∼…

2017 The Astrophysical Journal
eHST 77
A Measurement of the Galaxy Group-Thermal Sunyaev-Zel'dovich Effect Cross-Correlation Function
DOI: 10.1093/mnras/stw3311 Bibcode: 2017MNRAS.467.2315V

Jain, Bhuvnesh; Lidz, Adam; Vikram, Vinu

Stacking cosmic microwave background maps around known galaxy clusters and groups provides a powerful probe of the distribution of hot gas in these systems via the Sunyaev-Zel'dovich (SZ) effect. A stacking analysis allows one to detect the average SZ signal around low-mass haloes, to extend measurements out to large scales and measure the redshif…

2017 Monthly Notices of the Royal Astronomical Society
Planck 77
A uniform metallicity in the outskirts of massive, nearby galaxy clusters
DOI: 10.1093/mnras/stx1542 Bibcode: 2017MNRAS.470.4583U

Simionescu, A.; Allen, S. W.; Werner, N. +2 more

Suzaku measurements of a homogeneous metal distribution of Z ∼ 0.3 Solar in the outskirts of the nearby Perseus cluster suggest that chemical elements were deposited and mixed into the intergalactic medium before clusters formed, likely over 10 billion years ago. A key prediction of this early enrichment scenario is that the intracluster medium in…

2017 Monthly Notices of the Royal Astronomical Society
Suzaku 77
Asymptotic g modes: Evidence for a rapid rotation of the solar core
DOI: 10.1051/0004-6361/201730460 Bibcode: 2017A&A...604A..40F

Provost, J.; Corbard, T.; Turck-Chièze, S. +11 more

Context. Over the past 40 years, helioseismology has been enormously successful in the study of the solar interior. A shortcoming has been the lack of a convincing detection of the solar g modes, which are oscillations driven by gravity and are hidden in the deepest part of the solar body - its hydrogen-burning core. The detection of g modes is ex…

2017 Astronomy and Astrophysics
SOHO 77
Survey of Cold Water Lines in Protoplanetary Disks: Indications of Systematic Volatile Depletion
DOI: 10.3847/1538-4357/aa70ee Bibcode: 2017ApJ...842...98D

van Dishoeck, Ewine F.; Fedele, Davide; Lis, Dariusz C. +11 more

We performed very deep searches for 2 ground-state water transitions in 13 protoplanetary disks with the HIFI instrument on board the Herschel Space Observatory, with integration times up to 12 hr per line. We also searched for, with shallower integrations, two other water transitions that sample warmer gas. The detection rate is low, and the uppe…

2017 The Astrophysical Journal
Herschel 77
Chasing obscuration in type-I AGN: discovery of an eclipsing clumpy wind at the outer broad-line region of NGC 3783
DOI: 10.1051/0004-6361/201731175 Bibcode: 2017A&A...607A..28M

Kaastra, J. S.; Kriss, G. A.; Arav, N. +21 more

In 2016 we carried out a Swift monitoring programme to track the X-ray hardness variability of eight type-I AGN over a year. The purpose of this monitoring was to find intense obscuration events in AGN, and thereby study them by triggering joint XMM-Newton, NuSTAR, and HST observations. We successfully accomplished this for NGC 3783 in December 20…

2017 Astronomy and Astrophysics
XMM-Newton eHST 77
Evidence for a radiatively driven disc-wind in PDS 456?
DOI: 10.1093/mnrasl/slx129 Bibcode: 2017MNRAS.472L..15M

Tombesi, F.; Reeves, J. N.; Braito, V. +5 more

We present a newly discovered correlation between the wind outflow velocity and the X-ray luminosity in the luminous (Lbol ∼ 1047erg s - 1) nearby (z = 0.184) quasar PDS 456. All the contemporary XMM-Newton, NuSTAR and Suzaku observations from 2001-2014 were revisited and we find that the centroid energy of the blu…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 77
Extreme jet ejections from the black hole X-ray binary V404 Cygni
DOI: 10.1093/mnras/stx1048 Bibcode: 2017MNRAS.469.3141T

Gurwell, M.; Russell, D. M.; Fender, R. +14 more

We present simultaneous radio through sub-mm observations of the black hole X-ray binary (BHXB) V404 Cygni during the most active phase of its June 2015 outburst. Our 4 h long set of overlapping observations with the Very Large Array, the Sub-millimeter Array and the James Clerk Maxwell Telescope (SCUBA-2) covers eight different frequency bands (i…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 77
Luminosity dependence of the cyclotron line and evidence for the accretion regime transition in V 0332+53
DOI: 10.1093/mnras/stw3236 Bibcode: 2017MNRAS.466.2143D

Doroshenko, Victor; Tsygankov, Sergey S.; Mushtukov, Alexander A. +4 more

We report on the analysis of NuSTAR observations of the Be-transient X-ray pulsar V 0332+53 during the giant outburst in 2015 and another minor outburst in 2016. We confirm the cyclotron-line energy-luminosity correlation previously reported in the source and the line energy decrease during the giant outburst. Based on 2016 observations, we find t…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 77
Spectral Changes in the Hyperluminous Pulsar in NGC 5907 as a Function of Super-orbital Phase
DOI: 10.3847/1538-4357/834/1/77 Bibcode: 2017ApJ...834...77F

Harrison, F. A.; Stern, D.; Bachetti, M. +5 more

We present broadband, multi-epoch X-ray spectroscopy of the pulsating ultra-luminous X-ray source (ULX) in NGC 5907. Simultaneous XMM-Newton and NuSTAR data from 2014 are best described by a multicolor blackbody model with a temperature gradient as a function of accretion disk radius significantly flatter than expected for a standard thin accretio…

2017 The Astrophysical Journal
XMM-Newton 77