Search Publications

Deflections of Fast Coronal Mass Ejections and the Properties of Associated Solar Energetic Particle Events
DOI: 10.1088/0004-637X/754/2/100 Bibcode: 2012ApJ...754..100K

Gopalswamy, N.; Kahler, S. W.; Akiyama, S.

The onset times and peak intensities of solar energetic particle (SEP) events at Earth have long been thought to be influenced by the open magnetic fields of coronal holes (CHs). The original idea was that a CH lying between the solar SEP source region and the magnetic footpoint of the 1 AU observer would result in a delay in onset and/or a decrea…

2012 The Astrophysical Journal
SOHO 13
Observation of High-speed Outflows in Coronal Loops Associated with Photospheric Magnetic Field Evolution
DOI: 10.1088/0004-637X/760/1/82 Bibcode: 2012ApJ...760...82S

Liu, Y.; Su, J. T.; Liu, S. +2 more

Using SDO/AIA instruments, we provide an EUV observation of two adjacent loop strands (Loops 1 and 2) with one side of their footpoints rooted in the boundaries of active region (AR) NOAA 11158 and the other side in the quiet-Sun regions. The AR footpoints of Loop 1 were located in monopolar magnetic areas and those of Loop 2 in mixed polar areas …

2012 The Astrophysical Journal
Hinode 13
Titan airglow during eclipse
DOI: 10.1029/2012GL053230 Bibcode: 2012GeoRL..3918204W

Strobel, D. F.; West, R. A.; Gladstone, G. R. +4 more

Solar XUV photons can provide enough energy to account for the observed nitrogen UV dayglow emissions above 800 km, but a small or sporadic contribution from energetic particles cannot be ruled out. Furthermore, ion production at altitudes deeper than 800 km as inferred from radio occultation cannot be produced by solar XUV stimulation and implies…

2012 Geophysical Research Letters
Cassini 13
Blending of Cepheids in M33
DOI: 10.1088/0004-6256/144/4/113 Bibcode: 2012AJ....144..113C

Macri, Lucas M.; Pellerin, Anne; Chavez, Joy M.

A precise and accurate determination of the Hubble constant based on Cepheid variables requires proper characterization of many sources of systematic error. One of these is stellar blending, which biases the measured fluxes of Cepheids and the resulting distance estimates. We study the blending of 149 Cepheid variables in M33 by matching archival …

2012 The Astronomical Journal
eHST 13
External triggering of plasmoid development at Saturn
DOI: 10.1029/2012JA017625 Bibcode: 2012JGRA..117.7206K

Winglee, R. M.; Paty, C. S.; Harnett, E. M. +1 more

The Cassini spacecraft has encountered multiple plasmoids in Saturn's magnetotail thought to be produced by tail reconnection. However, single spacecraft measurements make it difficult to determine plasmoid size, where they form, the composition, and the geometry of the plasma sheet when plasmoids are produced. This paper examines these issues usi…

2012 Journal of Geophysical Research (Space Physics)
Cassini 13
A close look at the Centaurus A group of galaxies. IV. Recent star formation histories of late-type dwarfs around CenA
DOI: 10.1051/0004-6361/201218898 Bibcode: 2012A&A...541A.131C

Crnojević, D.; Grebel, E. K.; Cole, A. A.


Aims: We study a sample of five dwarf irregular galaxies in the CenA/M 83 group, which are companions to the giant elliptical CenA. We aim at deriving their physical properties over their lifetime and compare them to those of dwarfs located in different environments.
Methods: We use archival HST/ACS data and apply synthetic color-magnitu…

2012 Astronomy and Astrophysics
eHST 13
Analytical shear and flexion of Einasto dark matter haloes
DOI: 10.1051/0004-6361/201219539 Bibcode: 2012A&A...546A..32R

Baes, M.; Frutos-Alfaro, F.; Retana-Montenegro, E.

N-body simulations predict that dark matter haloes are described by specific density profiles on both galactic- and cluster-sized scales. Weak gravitational lensing through the measurements of their first and second order properties, shear and flexion, is a powerful observational tool for investigating the true shape of these profiles. One of the …

2012 Astronomy and Astrophysics
eHST 13
Regolith grain sizes of Saturn’s rings inferred from Cassini-CIRS far-infrared spectra
DOI: 10.1016/j.icarus.2012.09.012 Bibcode: 2012Icar..221..888M

Spilker, Linda; Morishima, Ryuji; Edgington, Scott G.

We analyze far-infrared (10-650 cm-1) emissivity spectra of Saturn’s main rings obtained by the Cassini Composite Infrared Spectrometer (CIRS). In modeling of the spectra, the single scattering albedos of regolith grains are calculated using the Mie theory, diffraction is removed with the delta-Eddington approximation, and the hemispher…

2012 Icarus
Cassini 13
A planetary companion around the K giant ɛ Corona Borealis
DOI: 10.1051/0004-6361/201219347 Bibcode: 2012A&A...546A...5L

Lee, B. -C.; Park, M. -G.; Han, I. +2 more


Aims: Our aim is to search for and study the origin of the low-amplitude and long-periodic radial velocity (RV) variations in K giants.
Methods: We present high-resolution RV measurements of K2 giant ɛ CrB from February 2005 to January 2012 using the fiber-fed Bohyunsan Observatory Echelle Spectrograph (BOES) at the Bohyunsan Optical Ast…

2012 Astronomy and Astrophysics
Hipparcos 13
The Merger History, Active Galactic Nucleus, and Dwarf Galaxies of Hickson Compact Group 59
DOI: 10.1088/0004-637X/745/1/30 Bibcode: 2012ApJ...745...30K

Hornschemeier, A. E.; Brandt, W. N.; Konstantopoulos, I. S. +16 more

Compact group galaxies often appear unaffected by their unusually dense environment. Closer examination can, however, reveal the subtle, cumulative effects of multiple galaxy interactions. Hickson Compact Group (HCG) 59 is an excellent example of this situation. We present a photometric study of this group in the optical (Hubble Space Telescope), …

2012 The Astrophysical Journal
eHST 13