Search Publications

Dynamics of a Prominence-horn Structure during Its Evaporation in the Solar Corona
DOI: 10.3847/2041-8205/827/2/L33 Bibcode: 2016ApJ...827L..33W

Liu, Wei; Li, Xing; Chen, Yao +3 more

The physical connections among and formation mechanisms of various components of the prominence-horn cavity system remain elusive. Here we present observations of such a system, focusing on a section of the prominence that rises and separates gradually from the main body. This forms a configuration sufficiently simple to yield clues regarding the …

2016 The Astrophysical Journal
SOHO 17
Identification of z ≳ 2 Herschel 500 µM Sources Using Color Deconfusion
DOI: 10.3847/0067-0049/222/1/4 Bibcode: 2016ApJS..222....4S

Elbaz, D.; Ferguson, H. C.; Leiton, R. +19 more

We present a new method to search for candidate z ≳ 2 Herschel 500 µm sources in the Great Observatories Origins Deep Survey-North field using a S500 µm/S24 µm “color deconfusion” technique. Potential high-z sources are selected against low-redshift ones from their large 500 to 24 µm flux density ratio…

2016 The Astrophysical Journal Supplement Series
Herschel 17
Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
DOI: 10.3847/1538-4357/833/2/224 Bibcode: 2016ApJ...833..224C

Baum, Stefi A.; O'Dea, Christopher P.; Cooke, Kevin C. +3 more

We present a multi-wavelength photometric and spectroscopic study of 42 Brightest Cluster Galaxies (BCGs) in two samples of galaxy clusters chosen for a gravitational lensing study. The study’s initial sample combines 25 BCGs from the Cluster Lensing and Supernova Survey with Hubble sample and 37 BCGs from the Sloan Giant Arcs Survey with a total …

2016 The Astrophysical Journal
Herschel eHST 17
Evolution of active region outflows throughout an active region lifetime
DOI: 10.1051/0004-6361/201628421 Bibcode: 2016A&A...594A..40Z

Poletto, G.; Zangrilli, L.

Context. We have shown previously that SOHO/UVCS data allow us to detect active region (AR) outflows at coronal altitudes higher than those reached by other instrumentation. These outflows are thought to be a component of the slow solar wind.
Aims: Our purpose is to study the evolution of the outflows in the intermediate corona from AR 8100, …

2016 Astronomy and Astrophysics
SOHO 17
The Environment of z > 1 3CR Radio Galaxies and QSOs: From Proto-clusters to Clusters of Galaxies?
DOI: 10.3847/0004-637X/826/1/46 Bibcode: 2016ApJ...826...46K

Macchetto, F. D.; Capetti, A.; Sparks, W. B. +8 more

We study the cluster environment for a sample of 21 radio loud active galactic nuclei from the 3CR catalog at z\gt 1, 12 radio galaxies (RGs) and nine quasars, with Hubble Space Telescope (HST) images in the optical and IR. We use two different approaches to determine cluster candidates. We identify the early-type galaxies (ETGs) in every field by…

2016 The Astrophysical Journal
eHST 17
How unusual is the cool-core radio halo cluster CL1821+643?
DOI: 10.1093/mnras/stw796 Bibcode: 2016MNRAS.459.2940K

Kale, Ruta; Parekh, Viral

Massive galaxy clusters with cool cores typically host diffuse radio sources called mini-haloes, whereas, those with non-cool cores host radio haloes. We attempt to understand the unusual nature of the cool-core galaxy cluster CL1821+643, which hosts a megaparsec-scale radio halo, using new radio observations and morphological analysis of its intr…

2016 Monthly Notices of the Royal Astronomical Society
Planck 17
Multi-wavelength properties of IGR J05007-7047 (LXP 38.55) and identification as a Be X-ray binary pulsar in the LMC
DOI: 10.1093/mnras/stw1408 Bibcode: 2016MNRAS.461.1875V

Haberl, F.; Udalski, A.; Sturm, R. +2 more

We report on the results of a ∼40-d multi-wavelength monitoring of the Be X-ray binary system IGR J05007-7047 (LXP 38.55). During that period the system was monitored in the X-rays using the Swift telescope and in the optical with multiple instruments. When the X-ray luminosity exceeded 1036 erg s-1 we triggered an XMM-Newton…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 17
Coalescence of magnetic flux ropes observed in the tailward high-speed flows
DOI: 10.1002/2016JA023526 Bibcode: 2016JGRA..12110898Z

Zhao, Yan; Yao, Zhonghua; Lu, Quanming +3 more

We report a tailward high-speed flow event observed by Cluster during 0203:00UT-0205:30UT on 20 September 2003. Within the flows, a series of three bipolar Bz signatures were observed. The first and third bipolar Bz signatures are identified as magnetic flux ropes, while the middle one is found to result from the collision of…

2016 Journal of Geophysical Research (Space Physics)
Cluster 17
Constraints on the H2O formation mechanism in the wind of carbon-rich AGB stars
DOI: 10.1051/0004-6361/201527049 Bibcode: 2016A&A...588A.124L

Blommaert, J. A. D. L.; De Ridder, J.; de Koter, A. +13 more

Context. The recent detection of warm H2O vapor emission from the outflows of carbon-rich asymptotic giant branch (AGB) stars challenges the current understanding of circumstellar chemistry. Two mechanisms have been invoked to explain warm H2O vapor formation. In the first, periodic shocks passing through the medium immediate…

2016 Astronomy and Astrophysics
Herschel ISO 17
The size and shape of the Milky Way disc and halo from M-type brown dwarfs in the BoRG survey
DOI: 10.1093/mnras/stw258 Bibcode: 2016MNRAS.458..425V

Trenti, M.; Bouwens, R. J.; Holwerda, B. W. +3 more

We have identified 274 M-type brown dwarfs in the Hubble Space Telescope's Wide Field Camera 3 pure parallel fields from the Brightest of Reionizing Galaxies (BoRG) survey for high-redshift galaxies. These are near-infrared observations with multiple lines of sight out of our Milky Way. Using these observed M-type brown dwarfs, we fitted a Galacti…

2016 Monthly Notices of the Royal Astronomical Society
eHST 17