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Proper motions for HST observations in three off-axis bulge fields
DOI: 10.1051/0004-6361/201117339 Bibcode: 2014A&A...562A..41S

Rich, R. M.; Soto, M.; Kuijken, K. +3 more


Aims: This is the second in a series of papers that attempt to unveil the kinematic structure of the Galactic bulge through studying radial velocities and proper motions. We report here ~15 000 new proper motions for three low foreground-extinction off-axis fields of the Galactic bulge.
Methods: Proper motions were derived from a combina…

2014 Astronomy and Astrophysics
eHST 15
Interesting Features in the Combined GALEX and Sloan Color Diagrams of Solar-like Galactic Populations
DOI: 10.1088/0004-6256/147/6/159 Bibcode: 2014AJ....147..159S

Smith, Myron A.; Bianchi, Luciana; Shiao, Bernard

We report on intriguing photometric properties of Galactic stars observed in the Galaxy Evolution Explorer (GALEX) satellite's far-UV (FUV) and near-UV (NUV) bandpasses, as well as from the ground-based Sloan Digital Sky Survey (SDSS) and the Kepler Input Catalog. The first property is that the (FUV - NUV) color distribution of stars in the Kepler…

2014 The Astronomical Journal
IUE 15
Suzaku Observation of IRAS 00521-7054, a Peculiar Type-II AGN with a Very Broad Feature at 6 keV
DOI: 10.1088/0004-637X/795/2/147 Bibcode: 2014ApJ...795..147R

Paltani, S.; Ricci, C.; Terashima, Y. +3 more

IRAS 00521-7054 is the first Seyfert 2 in which the presence of an extremely large Fe Kα line has been claimed. We report here on the analysis of a 100 ks Suzaku observation of the source. We confirm the existence of a very strong excess over the power-law X-ray continuum at E ~ 6 keV (EW ~= 800 eV), extending down to ~4.5 keV, and found that the …

2014 The Astrophysical Journal
Suzaku XMM-Newton 15
Analytical Solution for Waves in Planets with Atmospheric Superrotation. I. Acoustic and Inertia-Gravity Waves
DOI: 10.1088/0067-0049/213/1/17 Bibcode: 2014ApJS..213...17P

López-Valverde, M. A.; Imamura, T.; Peralta, J. +3 more

This paper is the first of a two-part study devoted to developing tools for a systematic classification of the wide variety of atmospheric waves expected on slowly rotating planets with atmospheric superrotation. Starting with the primitive equations for a cyclostrophic regime, we have deduced the analytical solution for the possible waves, simult…

2014 The Astrophysical Journal Supplement Series
VenusExpress 15
Understanding the dynamical structure of pulsating stars. HARPS spectroscopy of the δ Scuti stars ρ Puppis and DX Ceti
DOI: 10.1051/0004-6361/201322356 Bibcode: 2014A&A...561A.151N

Guiglion, G.; Poretti, E.; Rainer, M. +4 more

Context. High-resolution spectroscopy is a powerful tool to study the dynamical structure of a pulsating star's atmosphere.
Aims: We aim at comparing the line asymmetry and velocity of the two δ Sct stars ρ Pup and DX Cet with previous spectroscopic data obtained on classical Cepheids and β Cep stars.
Methods: We obtained, analysed and d…

2014 Astronomy and Astrophysics
Hipparcos 14
X-ray spectroscopy of the mixed morphology supernova remnant W 28 with XMM-Newton
DOI: 10.1093/pasj/psu031 Bibcode: 2014PASJ...66...62N

Ishida, Manabu; Bamba, Aya; Tatematsu, Ken'ichi +6 more

We report on spatially resolved X-ray spectroscopy of the north-eastern part of the mixed morphology supernova remnant (SNR) W 28 with XMM-Newton. The observed field of view includes a prominent and twisted shell emission forming the edge of this SNR as well as part of the center-filled X-ray emission brightening toward the south-west edge of the …

2014 Publications of the Astronomical Society of Japan
XMM-Newton 14
The Extreme Ultraviolet Deficit and Magnetically Arrested Accretion in Radio-loud Quasars
DOI: 10.1088/2041-8205/797/2/L33 Bibcode: 2014ApJ...797L..33P

Punsly, Brian

The Hubble Space Telescope composite quasar spectra presented in Telfer et al. show a significant deficit of emission in the extreme ultraviolet for the radio-loud component of the quasar population (RLQs) compared to the radio-quiet component of the quasar population. The composite quasar continuum emission between 1100 Å and ~580 Å is generally …

2014 The Astrophysical Journal
eHST 14
Non-minimal braneworld inflation after the Planck
DOI: 10.1007/s10509-013-1715-8 Bibcode: 2014Ap&SS.350..339N

Nozari, Kourosh; Rashidi, Narges

The recently released Planck data have constrained 4-dimensional inflationary parameters even more accurately than ever. We consider an extension of the braneworld model with induced gravity and a non-minimally coupled scalar field on the brane. We constraint the inflation parameters in this setup, by adopting six types of potential, in confrontat…

2014 Astrophysics and Space Science
Planck 14
A dynamical transition from atomic to molecular intermediate-velocity clouds
DOI: 10.1051/0004-6361/201322525 Bibcode: 2014A&A...564A..71R

Boulanger, F.; Lagache, G.; Kerp, J. +2 more

Context. Towards the high galactic latitude sky, the far-infrared (FIR) intensity is tightly correlated to the total hydrogen column density which is made up of atomic (H i) and molecular hydrogen (H2). Above a certain column density threshold, atomic hydrogen turns molecular.
Aims: We analyse gas and dust properties of intermediat…

2014 Astronomy and Astrophysics
Planck 14
First Extragalactic Detection of Submillimeter CH Rotational Lines from the Herschel Space Observatory
DOI: 10.1088/0004-637X/788/2/147 Bibcode: 2014ApJ...788..147R

Wilson, Christine D.; Glenn, Jason; Spinoglio, Luigi +5 more

We present the first extragalactic detections of several CH rotational transitions in the far-infrared in four nearby galaxies, NGC 1068, Arp 220, M82, and NGC 253, using the Herschel Space Observatory. The CH lines in all four galaxies are a factor of 2-4 brighter than the adjacent HCN and HCO+ J = 6-5 lines (also detected in the same …

2014 The Astrophysical Journal
Herschel 14