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Strong lensing in RX J1347.5-1145 revisited
DOI: 10.1093/mnras/stt2017 Bibcode: 2014MNRAS.437.1858K

Schmidt, R. W.; Köhlinger, F.

We present a revised strong lensing mass reconstruction of the galaxy cluster RX J1347.5-1145. The X-ray luminous cluster at redshift z = 0.451 has already been studied intensively in the past. Based on information of two such previous (strong-) lensing studies by Halkola et al. and Bradač et al., as well as by incorporating newly available data f…

2014 Monthly Notices of the Royal Astronomical Society
eHST 15
Dynamics and metallicity of far-infrared selected galaxies
DOI: 10.1093/mnras/stu1422 Bibcode: 2014MNRAS.443.3780W

Lutz, D.; Maiolino, R.; Marconi, A. +4 more

We present near-infrared integral field spectroscopy of 10 Herschel selected galaxies at z ∼ 1.5. From detailed mapping of the Hα and [N II] emission lines, we trace the dynamics, star formation rates, metallicities and also investigate gas fractions for these galaxies. For a few galaxies, the distribution of star formation as traced by Hα only tr…

2014 Monthly Notices of the Royal Astronomical Society
Herschel eHST 15
Automatic Tracking of Active Regions and Detection of Solar Flares in Solar EUV Images
DOI: 10.1007/s11207-013-0415-4 Bibcode: 2014SoPh..289.1643C

Caballero, C.; Aranda, M. C.

Solar catalogs are frequently handmade by experts using a manual approach or semi-automated approach. The appearance of new tools is very useful because the work is automated. Nowadays it is impossible to produce solar catalogs using these methods, because of the emergence of new spacecraft that provide a huge amount of information. In this articl…

2014 Solar Physics
SOHO 15
Orphan penumbrae: Submerging horizontal fields
DOI: 10.1051/0004-6361/201322340 Bibcode: 2014A&A...564A..91J

Bellot Rubio, L. R.; Jurčák, J.; Sobotka, M.


Aims: We investigate the properties of orphan penumbrae, which are photospheric filamentary structures observed in active regions near polarity inversion lines that resemble the penumbra of regular sunspots but are not connected to any umbra.
Methods: We use Hinode data from the Solar Optical Telescope to determine the properties of orph…

2014 Astronomy and Astrophysics
Hinode 15
Emission Measure Distribution for Diffuse Regions in Solar Active Regions
DOI: 10.1088/0004-637X/795/1/76 Bibcode: 2014ApJ...795...76S

Tripathi, Durgesh; Mason, Helen E.; Klimchuk, James A. +1 more

Our knowledge of the diffuse emission that encompasses active regions is very limited. In this paper we investigate two off-limb active regions, namely, AR 10939 and AR 10961, to probe the underlying heating mechanisms. For this purpose, we have used spectral observations from Hinode/EIS and employed the emission measure (EM) technique to obtain t…

2014 The Astrophysical Journal
Hinode 15
The evolving spectrum of the planetary nebula Hen 2-260
DOI: 10.1051/0004-6361/201322742 Bibcode: 2014A&A...567A..15H

Zijlstra, A. A.; van Hoof, P. A. M.; Hajduk, M. +3 more


Aims: We analysed the planetary nebula Hen 2-260 using optical spectroscopy and photometry. We compared our observations with the data from literature to search for evolutionary changes. We also searched for photomertic variability of the central star.
Methods: The object Hen 2-260 was observed with the SAAO 1.0 m telescope (photometry) …

2014 Astronomy and Astrophysics
eHST 15
Dayside/nightside asymmetry of ion densities and velocities in Saturn's inner magnetosphere
DOI: 10.1002/2014GL060229 Bibcode: 2014GeoRL..41.3717H

Wahlund, J. -E.; Morooka, M. W.; Holmberg, M. K. G.

We present Radio and Plasma Wave Science Langmuir probe measurements from 129 Cassini orbits, which show a day/night asymmetry in both ion density and ion velocity in the radial region 4-6 RS (1 RS = 60,268 km) from the center of Saturn. The ion densities ni vary from an average of ∼35 cm-3 around noon u…

2014 Geophysical Research Letters
Cassini 15
The candidate luminous blue variable G79.29+0.46: a comprehensive study of its ejecta through a multiwavelength analysis
DOI: 10.1093/mnras/stu296 Bibcode: 2014MNRAS.440.1391A

Umana, G.; Agliozzo, C.; Noriega-Crespo, A. +5 more

We present a multiwavelength analysis of the nebula around the candidate luminous blue variable G79.29+0.46. The study is based on our radio observations performed at the Expanded Very Large Array and at the Green Bank Telescope and on archival infrared data sets, including recent images obtained by the Herschel Space Observatory. We confirm that …

2014 Monthly Notices of the Royal Astronomical Society
Herschel ISO 15
CLASH: Extending Galaxy Strong Lensing to Small Physical Scales with Distant Sources Highly Magnified by Galaxy Cluster Members
DOI: 10.1088/0004-637X/786/1/11 Bibcode: 2014ApJ...786...11G

Infante, L.; Zheng, W.; Molino, A. +35 more

We present a complex strong lensing system in which a double source is imaged five times by two early-type galaxies. We take advantage in this target of the extraordinary multi-band photometric data set obtained as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) program, complemented by the spectroscopic measurements of the VL…

2014 The Astrophysical Journal
eHST 15
A state-of-the-art analysis of the dwarf irregular galaxy NGC 6822
DOI: 10.1051/0004-6361/201323075 Bibcode: 2014A&A...572A..26F

Hidalgo, S. L.; Bono, G.; Pietrinferni, A. +5 more

We present a detailed photometric study of the dwarf irregular galaxy NGC 6822 aimed at investigating the properties of its stellar populations and, in particular, the presence of stellar radial gradients. Our goal is to analyse the stellar populations in six fields, which cover the whole bar of this dwarf galaxy. We derived the quantitative star …

2014 Astronomy and Astrophysics
eHST 15