Search Publications

Chromophores from photolyzed ammonia reacting with acetylene: Application to Jupiter's Great Red Spot
DOI: 10.1016/j.icarus.2016.03.008 Bibcode: 2016Icar..274..106C

Baines, K. H.; Carlson, R. W.; Simon, A. A. +2 more

The high altitude of Jupiter's Great Red Spot (GRS) may enhance the upward flux of gaseous ammonia (NH3) into the high troposphere, where NH3 molecules can be photodissociated and initiate a chain of chemical reactions with downwelling acetylene molecules (C2H2). These reactions, experimentally studied e…

2016 Icarus
eHST 48
Warm absorbers in X-rays (WAX), a comprehensive high-resolution grating spectral study of a sample of Seyfert Galaxies - II. Warm absorber dynamics and feedback to galaxies
DOI: 10.1093/mnras/stw211 Bibcode: 2016MNRAS.457.3896L

Dewangan, Gulab C.; Guainazzi, Matteo; Laha, Sibasish +2 more

This paper is a sequel to the extensive study of warm absorber (WA) in X-rays carried out using high-resolution grating spectral data from XMM-Newton satellite (WAX-I). Here we discuss the global dynamical properties as well as the energetics of the WA components detected in the WAX sample. The slope of WA density profile (n ∝ r) esti…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 48
A free-form mass model of the Hubble Frontier Fields cluster AS1063 (RXC J2248.7-4431) with over one hundred constraints
DOI: 10.1093/mnras/stw865 Bibcode: 2016MNRAS.459.3447D

Broadhurst, Tom; Zheng, Wei; Lam, Daniel +5 more

We derive a free-form mass distribution for the massive cluster AS1063 (z = 0.348) using the completed optical imaging from the Hubble Frontier Fields programmme. Based on a subset of 11 multiply lensed systems with spectroscopic redshift, we produce a lens model that is accurate enough to secure new multiply lensed systems, totalling over a 100 a…

2016 Monthly Notices of the Royal Astronomical Society
eHST 48
The Complete Ultraviolet Spectrum of the Archetypal "Wind-dominated" Quasar Mrk 231: Absorption and Emission from a High-speed Dusty Nuclear Outflow
DOI: 10.3847/0004-637X/825/1/42 Bibcode: 2016ApJ...825...42V

Veilleux, S.; Rupke, D. S. N.; Hamann, F. +2 more

New near- and far-ultraviolet (NUV and FUV) Hubble Space Telescope spectra of Mrk 231, the nearest quasar known, are combined with ground-based optical spectra to study the remarkable dichotomy between the FUV and NUV-optical spectral regions in this object. The FUV emission-line features are faint, broad, and highly blueshifted (up to ∼7000 km s<…

2016 The Astrophysical Journal
eHST 48
Observation of a Quasiperiodic Pulsation in Hard X-Ray, Radio, and Extreme-ultraviolet Wavelengths
DOI: 10.3847/0004-637X/822/1/7 Bibcode: 2016ApJ...822....7K

Kumar, Pankaj; Cho, Kyung-Suk; Nakariakov, Valery M.

We present a multiwavelength analysis of a quasiperiodic pulsation (QPP) observed in the hard X-ray (HXR), radio, and extreme-ultraviolet (EUV) channels during an M1.9 flare that occurred on 2011 September 23-24. The nonthermal HXR emission in 25-50 keV observed by RHESSI shows five distinct impulsive peaks of decaying amplitude with a period of a…

2016 The Astrophysical Journal
Hinode 48
Nature, distribution, and origin of Titan's Undifferentiated Plains
DOI: 10.1016/j.icarus.2015.11.034 Bibcode: 2016Icar..270..162L

Janssen, M. A.; Cassini RADAR Team; Lopes, Rosaly M. C. +15 more

The Undifferentiated Plains on Titan, first mapped by Lopes et al. (Lopes, R.M.C. et al., 2010. Icarus, 205, 540-588), are vast expanses of terrains that appear radar-dark and fairly uniform in Cassini Synthetic Aperture Radar (SAR) images. As a result, these terrains are often referred to as ;blandlands;. While the interpretation of several other…

2016 Icarus
Cassini 48
The Search for Molecular Outflows in Local Volume AGNs with Herschel-PACS
DOI: 10.3847/0004-637X/826/2/111 Bibcode: 2016ApJ...826..111S

Sturm, E.; Veilleux, S.; González-Alfonso, E. +3 more

We present the results from a systematic search for galactic-scale, molecular (OH 119 µm) outflows in a sample of 52 Local Volume (d\lt 50 Mpc) Burst Alert Telescope detected active galactic nuclei (BAT AGNs) with Herschel-PACS. We combine the results from our analysis of the BAT AGNs with the published Herschel/PACS data of 43 nearby (z\lt …

2016 The Astrophysical Journal
Herschel 48
Cloud Structure of Galactic OB Cluster-forming Regions from Combining Ground- and Space-based Bolometric Observations
DOI: 10.3847/0004-637X/828/1/32 Bibcode: 2016ApJ...828...32L

Li, Di; Qian, Lei; Rosolowsky, Erik +13 more

We have developed an iterative procedure to systematically combine the millimeter and submillimeter images of OB cluster-forming molecular clouds, which were taken by ground-based (CSO, JCMT, APEX, and IRAM-30 m) and space telescopes (Herschel and Planck). For the seven luminous (L\gt {10}6 L ) Galactic OB cluster-forming mo…

2016 The Astrophysical Journal
Herschel Planck 48
Further ALMA observations and detailed modeling of the Red Rectangle
DOI: 10.1051/0004-6361/201628546 Bibcode: 2016A&A...593A..92B

Sánchez Contreras, C.; Alcolea, J.; Santander-García, M. +3 more


Aims: We aim to study the rotating and expanding gas in the Red Rectangle, which is a well known bipolar nebula surrounding a double stellar system whose primary is a post-asymptotic giant branch (post-AGB) star. We analyze the properties of both components and the relation between them. Rotating disks have been very elusive in post-AGB nebul…

2016 Astronomy and Astrophysics
Herschel eHST 48
Composition, seasonal change, and bathymetry of Ligeia Mare, Titan, derived from its microwave thermal emission
DOI: 10.1002/2015JE004920 Bibcode: 2016JGRE..121..233L

Lorenz, R. D.; Karatekin, O.; Janssen, M. A. +8 more

For the last decade, the passive radiometer incorporated in the Cassini RADAR has recorded the 2.2 cm wavelength thermal emission from Titan's seas. In this paper, we analyze the radiometry observations collected from February 2007 to January 2015 over one of these seas, Ligeia Mare, with the goal of providing constraints on its composition, bathy…

2016 Journal of Geophysical Research (Planets)
Cassini 48