Search Publications

VLBI Astrometry of the Semiregular Variable RX Bootis
DOI: 10.1093/pasj/64.1.7 Bibcode: 2012PASJ...64....7K

Tafoya, Daniel; Kurayama, Tomoharu; Honma, Mareki +10 more

We present distance measurements of the semiregular variable RX Bootis (RX Boo) with its annual parallax. Using the unique dual-beam system of the VLBI Exploration of Radio Astrometry (VERA) telescope, we conducted astrometric observations of a water maser spot accompanying RX Boo, referred to the quasar J1419+2706 separated by 1.°69 from RX Boo. …

2012 Publications of the Astronomical Society of Japan
Hipparcos 24
Discovery of the Most Isolated Globular Cluster in the Local Universe
DOI: 10.1088/2041-8205/751/1/L19 Bibcode: 2012ApJ...751L..19J

Lee, Myung Gyoon; Jang, In Sung; Lim, Sungsoon +1 more

We report the discovery of two new globular clusters in the remote halos of M81 and M82 in the M81 Group based on Hubble Space Telescope archive images. They are brighter than typical globular clusters (MV = -9.34 mag for GC-1 and MV = -10.51 mag for GC-2), and much larger than known globular clusters with similar luminosity …

2012 The Astrophysical Journal
eHST 24
Formulation of a wind specification for Titan late polar summer exploration
DOI: 10.1016/j.pss.2012.05.015 Bibcode: 2012P&SS...70...73L

Achterberg, Richard K.; Lorenz, Ralph D.; Tokano, Tetsuya +4 more

Titan's polar regions, and its hydrocarbon lakes in particular, are of interest for future exploration. The polar conditions have considerable seasonal variation and are distinct from the equatorial environment experienced by Huygens. Thus specific environmental models are required for these regions. This paper, informed by Cassini and groundbased…

2012 Planetary and Space Science
Cassini 24
Recurrent Radio Outbursts at the Center of the NGC 1407 Galaxy Group
DOI: 10.1088/0004-637X/755/2/172 Bibcode: 2012ApJ...755..172G

Raychaudhury, Somak; Clarke, Tracy E.; Giacintucci, Simona +6 more

We present deep Giant Metrewave Radio Telescope (GMRT) radio observations at 240, 330, and 610 MHz of the complex radio source at the center of the NGC 1407 galaxy group. Previous GMRT observations at 240 MHz revealed faint, diffuse emission enclosing the central twin-jet radio galaxy. This has been interpreted as an indication of two possible rad…

2012 The Astrophysical Journal
XMM-Newton 24
The Free Energy of NOAA Solar Active Region AR 11029
DOI: 10.1007/s11207-011-9878-3 Bibcode: 2012SoPh..276..133G

Leka, K. D.; Wheatland, M. S.; Gilchrist, S. A.

The NOAA active region (AR) 11029 was a small but highly active sunspot region which produced 73 GOES soft X-ray flares during its transit of the disk in late October 2009. The flares appear to show a departure from the well-known power law frequency-size distribution. Specifically, too few GOES C-class and no M-class flares were observed by compa…

2012 Solar Physics
Hinode 24
What are the physical mechanisms of eruptions and CMEs?
DOI: 10.1016/j.asr.2011.10.023 Bibcode: 2012AdSpR..49.1598S

Aulanier, Guillaume; Schmieder, Brigitte

CMEs are due to physical phenomena that drive both, eruptions and flares in active regions. Eruptions/CMEs must be driven from initially force-free current-carrying magnetic field. Twisted flux ropes, sigmoids, current lanes and pattern in photospheric current maps show a clear evidence of currents parallel to the magnetic field. Eruptions occur s…

2012 Advances in Space Research
SOHO 24
A Conditional Luminosity Function Model of the Cosmic Far-infrared Background Anisotropy Power Spectrum
DOI: 10.1088/0004-637X/760/1/14 Bibcode: 2012ApJ...760...14D

Cooray, Asantha; De Bernardis, Francesco

The cosmic far-infrared background (CFIRB) is expected to be generated by faint, dusty star-forming galaxies during the peak epoch of galaxy formation. The anisotropy power spectrum of the CFIRB captures the spatial distribution of these galaxies in dark matter halos and the spatial distribution of dark matter halos in the large-scale structure. E…

2012 The Astrophysical Journal
Herschel 24
The nuclear polycyclic aromatic hydrocarbon emission of merger system NGC 1614: rings within rings
DOI: 10.1111/j.1365-2966.2011.20186.x Bibcode: 2012MNRAS.420.2209V

Reunanen, Juha; Väisänen, Petri; Zijlstra, Albert A. +2 more

It is important to understand the interplay between nuclear star formation and nuclear activity when studying the evolution of gas-rich galaxy mergers. We present here new spatially resolved L-band integral field unit observations of the inner kpc of the luminous infrared galaxy NGC 1614. A broad ring of 3.3-µm polycyclic aromatic hydrocarbo…

2012 Monthly Notices of the Royal Astronomical Society
eHST 24
Turbulent Characteristics in the Intensity Fluctuations of a Solar Quiescent Prominence Observed by the Hinode Solar Optical Telescope
DOI: 10.1088/0004-637X/745/2/185 Bibcode: 2012ApJ...745..185L

Foullon, C.; Chapman, S. C.; Leonardis, E.

We focus on Hinode Solar Optical Telescope (SOT) calcium II H-line observations of a solar quiescent prominence (QP) that exhibits highly variable dynamics suggestive of turbulence. These images capture a sufficient range of scales spatially (~0.1-100 arcsec) and temporally (~16.8 s-4.5 hr) to allow the application of statistical methods used to q…

2012 The Astrophysical Journal
Hinode 24
Tidal control of jet eruptions on Enceladus as observed by Cassini ISS between 2005 and 2007
DOI: 10.1016/j.icarus.2012.06.022 Bibcode: 2012Icar..220..896H

Spitale, J. N.; Helfenstein, P.; Hurford, T. A.

Observations of Enceladus have revealed active jets of material erupting from cracks on its south polar surface. It has previously been proposed that diurnal tidal stress, driven by Enceladus' orbital eccentricity, may actively produce surface movement along these cracks daily and thus may regulate when eruptions occur. Our analysis of the stress …

2012 Icarus
Cassini 24