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An interferometric study of the post-AGB binary 89 Herculis. II. Radiative transfer models of the circumbinary disk
DOI: 10.1051/0004-6361/201423749 Bibcode: 2014A&A...568A..12H

Regibo, S.; Wevers, T.; Verhoelst, T. +6 more

Context. The presence of stable disks around post-asymptotic giant branch (post-AGB) binaries is a widespread phenomenon. Also, the presence of (molecular) outflows is now commonly inferred in these systems.
Aims: In the first paper of this series, a surprisingly large fraction of optical light was found to be resolved in the 89 Her post-AGB …

2014 Astronomy and Astrophysics
Herschel ISO 38
A Comparison of X-Ray and Optical Emission in Cassiopeia A
DOI: 10.1088/0004-637X/789/2/138 Bibcode: 2014ApJ...789..138P

Fesen, Robert A.; Patnaude, Daniel J.

Broadband optical and narrowband Si XIII X-ray images of the young Galactic supernova remnant Cassiopeia A (Cas A) obtained over several decades are used to investigate spatial and temporal emission correlations on both large and small angular scales. The data examined consist of optical and near-infrared ground-based and Hubble Space Telescope im…

2014 The Astrophysical Journal
eHST 38
The radial gradient of the near-surface shear layer of the Sun
DOI: 10.1051/0004-6361/201424839 Bibcode: 2014A&A...570L..12B

Schou, J.; Gizon, L.; Barekat, A.

Context. Helioseismology has provided unprecedented information about the internal rotation of the Sun. One of the important achievements was the discovery of two radial shear layers: one near the bottom of the convection zone (the tachocline) and one near the surface. These shear layers may be important ingredients for explaining the magnetic cyc…

2014 Astronomy and Astrophysics
SOHO 38
Determining Inclinations of Active Galactic Nuclei via Their Narrow-line Region Kinematics. II. Correlation with Observed Properties
DOI: 10.1088/0004-637X/785/1/25 Bibcode: 2014ApJ...785...25F

Turner, T. J.; Kraemer, S. B.; Crenshaw, D. M. +2 more

Active galactic nuclei (AGNs) are axisymmetric systems to first order; their observed properties are likely strong functions of inclination with respect to our line of sight, yet the specific inclinations of all but a few AGNs are generally unknown. By determining the inclinations and geometries of nearby Seyfert galaxies using the kinematics of t…

2014 The Astrophysical Journal
eHST 38
Compilation of Catalog of Stellar Equatorial Coordinates and B-Magnitudes Using UKRVO Plate Database
Bibcode: 2014OAP....27...53A

Pakuliak, L. K.; Yatsenko, A. I.; Shatokhina, S. V. +6 more

To ensure the rational use of informational resources generated by UkrVO in MAO NASU, a catalog of equatorial coordinates (α, δ) and B-magnitudes of stars was created by using plates obtained during observational campaign named FON (ukr., Photographic Sky Survey). 102 plates with field of view of 8° were processed. Digitization of plates with size…

2014 Odessa Astronomical Publications
Hipparcos 38
Solar Polar Fields and the 22-Year Activity Cycle: Observations and Models
DOI: 10.1007/s11214-014-0064-4 Bibcode: 2014SSRv..186..325P

Petrie, G. J. D.; Petrovay, K.; Schatten, K.

We explore observations and models of the interacting, cyclical behavior of the active regions and the polar magnetic fields of the Sun. We focus on observational evidence of these fields interacting across the corridor between active and polar latitudes. We present observations of diverse magnetic signatures on, above and beneath the solar surfac…

2014 Space Science Reviews
SOHO 38
Reversal or no reversal: the evolution of the star formation rate-density relation up to z ∼ 1.6
DOI: 10.1093/mnras/stt1901 Bibcode: 2014MNRAS.437..458Z

Finoguenov, A.; Berta, S.; Magnelli, B. +27 more

We investigate the evolution of the star formation rate (SFR)-density relation in the Extended Chandra Deep Field South and the Great Observatories Origin Deep Survey fields up to z ∼ 1.6. In addition to the `traditional method', in which the environment is defined according to a statistical measurement of the local galaxy density, we use a `dynam…

2014 Monthly Notices of the Royal Astronomical Society
Herschel 38
Hubble Space Telescope Near-ultraviolet Spectroscopy of the Bright CEMP-no Star BD+44°493
DOI: 10.1088/0004-637X/790/1/34 Bibcode: 2014ApJ...790...34P

Smith, Verne V.; Beers, Timothy C.; Placco, Vinicius M. +10 more

We present an elemental-abundance analysis, in the near-ultraviolet (NUV) spectral range, for the extremely metal-poor star BD+44°493 a ninth magnitude subgiant with [Fe/H] =-3.8 and enhanced carbon, based on data acquired with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope. This star is the brightest example of a class of …

2014 The Astrophysical Journal
eHST 38
Plasma flows in Saturn's nightside magnetosphere
DOI: 10.1002/2014JA019912 Bibcode: 2014JGRA..119.4521T

Thomsen, M. F.; Wilson, R. J.; Tokar, R. L. +1 more

The plasma properties, especially the flow parameters, obtained from numerical integration of Cassini Plasma Spectrometer (CAPS) Ion Mass Spectrometer measurements during intervals when the CAPS field of view encompassed both inward and outward flow directions relative to corotation are examined for nightside data (18-06 local time) during 2006, 2…

2014 Journal of Geophysical Research (Space Physics)
Cassini 38
Vertical velocities from proper motions of red clump giants
DOI: 10.1051/0004-6361/201424573 Bibcode: 2014A&A...572A.101L

López-Corredoira, M.; Figueras, F.; Garzón, F. +1 more


Aims: We derive the vertical velocities of disk stars in the range of Galactocentric radii of R = 5 - 16 kpc within 2 kpc in height from the Galactic plane. This kinematic information is connected to dynamical aspects in the formation and evolution of the Milky Way, such as the passage of satellites and vertical resonance and determines wheth…

2014 Astronomy and Astrophysics
Gaia 38