Search Publications

Width of Radio-Loud and Radio-Quiet CMEs
DOI: 10.1007/s11207-007-9062-y Bibcode: 2007SoPh..246..409M

Gopalswamy, N.; Michalek, G.; Xie, H.

In the present paper we report on the difference in angular sizes between radio-loud and radio-quiet CMEs. For this purpose we compiled these two samples of events using Wind/WAVES and SOHO/LASCO observations obtained during 1996 - 2005. We show that the radio-loud CMEs are almost twice as wide as the radio-quiet CMEs (considering expanding parts …

2007 Solar Physics
SOHO 23
The velocity structure of moving magnetic feature pairs around sunspots: support for the U-loop model
DOI: 10.1051/0004-6361:20077900 Bibcode: 2007A&A...471.1035Z

Woch, J.; Solanki, S. K.; Zhang, J. +1 more

Context: Moving magnetic feature (MMF) pairs are among the most significant fine-scale structures around sunspots. Several models have been proposed to interpret the origin and evolution of MMF pairs. These models provide important clues to understanding MMF pairs.
Aims: We present an analysis of the velocity structure of MMF pairs in order to…

2007 Astronomy and Astrophysics
SOHO 23
Optical colours of AGN in the extended Chandra deep field South: obscured black holes in early type galaxies
DOI: 10.1051/0004-6361:20077651 Bibcode: 2007A&A...475..115R

Georgantopoulos, I.; Rovilos, E.

We investigate the optical colours of X-ray sources from the Extended Chandra Deep Field South (ECDFS) using photometry from the COMBO-17 survey, aiming to explore AGN - galaxy feedback models. The X-ray sources populate both the “blue” and the “red sequence” on the colour-magnitude diagram. However, sources in the “red sequence” appear systematic…

2007 Astronomy and Astrophysics
eHST 23
Rosetta Asteroid Targets: 2867 Steins and 21 Lutetia
DOI: 10.1007/s11214-006-9029-6 Bibcode: 2007SSRv..128...67B

Barucci, M. A.; Rossi, A.; Fulchignoni, M.

In preparation for the flyby of the Rosetta spacecraft, the state of the knowledge of 21 Lutetia and 2867 Steins obtained by ground based observations is reported. Preliminary determination of shape and/or size, rotational properties and taxonomic types are presented for both asteroids. The dusty environment of the targets has been studied in orde…

2007 Space Science Reviews
Rosetta 23
Cool Customers in the Stellar Graveyard. IV. Spitzer Search for Mid-IR excesses Around Five DAs
DOI: 10.1086/521394 Bibcode: 2007AJ....134.1662D

Debes, John H.; Sigurdsson, Steinn; Hansen, Brad

Hydrogen atmosphere white dwarfs with metal lines, so-called DAZs, require external accretion of material to explain the presence of weak metal-line absorption in their photospheres. The source of this material is currently unknown, but could come from the interstellar medium, unseen companions, or relic planetesimals from asteroid belt or Kuiper …

2007 The Astronomical Journal
eHST 23
An Update on the X-Ray Transient Narrow-Line Seyfert 1 Galaxy WPVS 007: Swift Observations of UV Variability and Persistence of X-Ray Faintness
DOI: 10.1086/513072 Bibcode: 2007AJ....133.1988G

O'Brien, Paul T.; Schady, Patricia; Leighly, Karen M. +3 more

We report on the detection of UV variability and the persistence of X-ray faintness of the X-ray transient narrow-line Seyfert 1 galaxy WPVS 007 based on the first year of monitoring with Swift between 2005 October and 2007 January. WPVS 007 has been an unusual source. Although it was X-ray-bright in the ROSAT All-Sky Survey, it has been extremely…

2007 The Astronomical Journal
IUE eHST 23
0.5 Mpc-scale extended X-ray emission in the z = 2.48 radio galaxy 4C 23.56
DOI: 10.1111/j.1365-2966.2006.11358.x Bibcode: 2007MNRAS.376..151J

Dunlop, J.; Almaini, O.; Best, P. N. +1 more

We present an XMM-Newton observation of the radio galaxy 4C 23.56 at z = 2.48 which reveals extended X-ray emission coincident with the radio lobes spanning ~0.5 Mpc. These are the largest X-ray-bright lobes known at z > 2. Under the assumption that these features result from inverse-Compton scattering of cosmic microwave background photons by …

2007 Monthly Notices of the Royal Astronomical Society
XMM-Newton 23
The Effects of Polarization Crosstalk and Solar Rotation on Measuring Full-Disk Solar Photospheric Vector Magnetic Fields
DOI: 10.1086/520056 Bibcode: 2007ApJ...666..559S

Zhang, H. Q.; Su, J. T.

Observations of full-disk solar photospheric vector magnetic fields are very important for the studies of the global properties and evolution of solar magnetism. Such observations can allow us to investigate the magnetic connectivities between active regions and the nonpotentiality of magnetic fields with a much wider field of view (FOV) than do l…

2007 The Astrophysical Journal
SOHO 23
Are supergranule sizes anti-correlated with magnetic activity?
DOI: 10.1051/0004-6361:20066644 Bibcode: 2007A&A...466.1123M

Meunier, N.; Roudier, T.; Tkaczuk, R.

Context: The variation of supergranule cell sizes with the magnetic environment is still controversial.
Aims: We study this relation in detail to understand the discrepancies observed between previous results.
Methods: We determine the cell size using divergence of horizontal flows derived from local correlation tracking of intensity maps …

2007 Astronomy and Astrophysics
SOHO 23
Breakdown of the frozen-in condition in the Earth's magnetotail
DOI: 10.1029/2006JA012000 Bibcode: 2007JGRA..112.4215L

RèMe, H.; Owen, C. J.; Dunlop, M. W. +3 more

We investigate in detail the breakdown of the frozen-in condition detected by Cluster at the downstream distance of ∼19 RE in the midnight sector of the magnetotail during a substorm expansion on 22 August 2001. It is found that the breakdown occurred (1) in a low-density environment with moderate to large proton plasma flow and signifi…

2007 Journal of Geophysical Research (Space Physics)
Cluster 23