Search Publications

Non-thermal "Burst-on-Tail" of Long-Duration Solar Event on 26 October 2003
DOI: 10.1007/s11207-012-0112-8 Bibcode: 2012SoPh..281..749Z

Struminsky, A.; Zimovets, I.

Observations of a rare long-duration solar event of GOES class X1.2 from 26 October 2003 are presented. This event showed a pronounced burst of hard X-ray and microwave emission, which was extremely delayed (> 60 min) with respect to the main impulsive phase and did not have any significant response visible in soft X-ray emission. We refer to t…

2012 Solar Physics
INTEGRAL SOHO 14
Extranuclear Hα-emitting complexes in low-z (U)LIRGs: precursors of tidal dwarf galaxies?
DOI: 10.1051/0004-6361/201117438 Bibcode: 2012A&A...538A..61M

Colina, L.; Arribas, S.; Miralles-Caballero, D.

This paper characterizes the physical and kinematic properties of external massive star-forming regions in a sample of (U)LIRGs. We use high angular resolution ACS images from the Hubble Space Telescope (HST) in F435W (~B) and F814W (~I) bands, as well as Hα -line emission maps obtained with integral field spectroscopy. We find 31 external Hα -emi…

2012 Astronomy and Astrophysics
eHST 14
The radio spectra of reddened Two Micron All Sky Survey quasi-stellar objects: evidence for young radio jets
DOI: 10.1111/j.1365-2966.2012.20446.x Bibcode: 2012MNRAS.421.2223G

Georgakakis, A.; Hopkins, A. M.; Afonso, J. +1 more

Multifrequency radio continuum observations (1.4-22 GHz) of a sample of reddened quasi-stellar objects (QSOs) are presented. We find a high incidence (13/16) of radio spectral properties, such as low-frequency turnovers, high-frequency spectral breaks or steep power-law slopes, similar to those observed in powerful compact steep spectrum (CSS) and…

2012 Monthly Notices of the Royal Astronomical Society
eHST 14
Correlations Between CME Parameters and Sunspot Activity
DOI: 10.1007/s11207-011-9925-0 Bibcode: 2012SoPh..278..203D

Du, Zhanle

Smoothed monthly mean coronal mass ejection (CME) parameters (speed, acceleration, central position angle, angular width, mass, and kinetic energy) for Cycle 23 are cross-analyzed, showing that there is a high correlation between most of them. The CME acceleration (a) is highly correlated with the reciprocal of its mass (M), with a correlation coe…

2012 Solar Physics
SOHO 14
Magnetic field amplification in electron phase-space holes and related effects
DOI: 10.5194/angeo-30-711-2012 Bibcode: 2012AnGeo..30..711T

Baumjohann, W.; Treumann, R. A.

Three-dimensional electron phase-space holes are shown to have positive charges on the plasma background, which produce a radial electric field and force the trapped electron component into an azimuthal drift. In this way electron holes generate magnetic fields in the hole. We solve the cylindrical hole model exactly for the hole charge, electric …

2012 Annales Geophysicae
Cluster 14
Evolution in the Dust Lane Fraction of Edge-on L* V Spiral Galaxies Since z = 0.8
DOI: 10.1088/0004-637X/753/1/25 Bibcode: 2012ApJ...753...25H

Dalcanton, J. J.; Koekemoer, A.; Böker, T. +5 more

The presence of a well-defined and narrow dust lane in an edge-on spiral galaxy is the observational signature of a thin and dense molecular disk, in which gravitational collapse has overcome turbulence. Using a sample of galaxies out to z ~ 1 extracted from the COSMOS survey, we identify the fraction of massive (L* V ) disks that displ…

2012 The Astrophysical Journal
eHST 14
Unusual Stokes V profiles during flaring activity of a delta sunspot
DOI: 10.1051/0004-6361/201219272 Bibcode: 2012A&A...547A..34F

Fletcher, L.; Snik, F.; Fischer, C. E. +2 more


Aims: We analyze a set of full Stokes profile observations of the flaring active region NOAA 10808. The region was recorded with the Vector-Spectromagnetograph of the Synoptic Optical Long-term Investigations of the Sun facility. The active region produced several successive X-class flares between 19:00 UT and 24:00 UT on September 13, 2005 a…

2012 Astronomy and Astrophysics
SOHO 14
The relation between surface star formation rate density and spiral arms in NGC 5236 (M 83)
DOI: 10.1051/0004-6361/201117432 Bibcode: 2012A&A...537A.145S

Larsen, S. S.; Silva-Villa, E.

Context. For a long time the consensus has been that star formation rates are higher in the interior of spiral arms in galaxies, compared to inter-arm regions. However, recent studies have found that the star formation inside the arms is not more efficient than elsewhere in the galaxy. Previous studies have based their conclusion mainly on integra…

2012 Astronomy and Astrophysics
eHST 14
A Catalog of Galactic Infrared Carbon Stars
DOI: 10.1088/0004-6256/143/2/36 Bibcode: 2012AJ....143...36C

Chen, P. S.; Yang, X. H.

We collected almost all of the Galactic infrared carbon stars (IRCSs) from literature published up to the present to organize a catalog of 974 Galactic IRCSs in this paper. Some of their photometric properties in the near-, mid-, and far-infrared are discussed.

2012 The Astronomical Journal
AKARI 14
Kinematics and Flare Properties of Radio-Loud CMEs
DOI: 10.1007/s11207-012-0111-9 Bibcode: 2012SoPh..281..765P

Prakash, O.; Shanmugaraju, A.; Umapathy, S. +1 more

A detailed analysis of the characteristics of coronal mass ejections (CMEs) and flares associated with decameter-hectometer wavelength type-II radio bursts (hereafter DH-type-II radio bursts, DH-CMEs or radio-loud CMEs) observed in the period 1997 - 2008 is presented. A sample of 61 limb events is divided into two populations based on the residual…

2012 Solar Physics
SOHO 14