Search Publications

Near-infrared imaging polarimetry of young stellar objects in ρ Ophiuchi
DOI: 10.1111/j.1365-2966.2007.12715.x Bibcode: 2008MNRAS.384..907B

Gledhill, T. M.; Lucas, P. W.; Beckford, A. F. +1 more

The results of a near-infrared (J H K LP) imaging linear polarimetry survey of 20 young stellar objects (YSOs) in ρ Ophiuchi are presented. The majority of the sources are unresolved, with K-band polarizations, PK < 6 per cent. Several objects are associated with extended reflection nebulae. These objects have centrosymmet…

2008 Monthly Notices of the Royal Astronomical Society
eHST 20
Evidence for metallicity spreads in three massive M 31 globular clusters
DOI: 10.1051/0004-6361:20078899 Bibcode: 2008A&A...483..769F

Jablonka, P.; Sarajedini, A.; Meylan, G. +3 more

Aims: We quantify the intrinsic width of the red giant branches of three massive globular clusters in M 31 in a search for metallicity spreads within these objects.
Methods: We present HST/ACS observations of three massive clusters in M 31, G78, G213, and G280. A thorough description of the photometry extraction and calibration is presented. A…

2008 Astronomy and Astrophysics
eHST 20
High-resolution Enceladus atlas derived from Cassini-ISS images
DOI: 10.1016/j.pss.2007.03.014 Bibcode: 2008P&SS...56..109R

Scholten, F.; Matz, K. -D.; Neukum, G. +8 more

The Cassini Imaging Science Subsystem (ISS) acquired 377 high-resolution images (<1 km/pixel) during three close flybys of Enceladus in 2005 [Porco, C.C., et al., 2006. Cassini observes the active south pole of Enceladus. Science 311, 1393-1401.]. We combined these images with lower resolution Cassini images and four others taken by Voyager cam…

2008 Planetary and Space Science
Cassini 20
A reinterpretation of the energy balance in active region loops following new results from Hinode EIS
DOI: 10.1051/0004-6361:200809847 Bibcode: 2008A&A...486L...5B

Bradshaw, S. J.

Context: New observations made by the Hinode EUV Imaging Spectrometer have revealed persistent redshifts in solar active region loops in the temperature range 105.6 ≤ T ≤ 106.4 K. The presence of redshifts, interpreted as bulk downflows, indicates that the loops are undergoing radiative cooling rather than continuous heating.…

2008 Astronomy and Astrophysics
Hinode 20
Segmentation of extreme ultraviolet solar images via multichannel fuzzy clustering
DOI: 10.1016/j.asr.2007.10.021 Bibcode: 2008AdSpR..42..917B

Hochedez, Jean-François; Delouille, Véronique; Barra, Vincent

The study of the variability of the solar corona and the monitoring of its traditional regions (Coronal Holes, Quiet Sun and Active Regions) are of great importance in astrophysics as well as in view of the Space Weather and Space Climate applications. Here we propose a multichannel unsupervised spatially constrained fuzzy clustering algorithm tha…

2008 Advances in Space Research
SOHO 20
Inverse Compton emission from the lobes of 3C353
DOI: 10.1111/j.1365-2966.2008.13028.x Bibcode: 2008MNRAS.386..337G

Hardcastle, M. J.; Croston, J. H.; Perley, R. A. +2 more

X-ray emission due to inverse Compton scattering of microwave background photons by electrons in the lobes of powerful radio galaxies has now been seen in a large number of objects. Combining an inverse Compton model for the lobe X-ray emission with information obtained from radio synchrotron emission provides a method of constraining the electron…

2008 Monthly Notices of the Royal Astronomical Society
XMM-Newton 20
The Plasma Structure of the Southwestern Region of the Cygnus Loop with the XMM-Newton Observatory
DOI: 10.1086/592398 Bibcode: 2008ApJ...688.1102U

Katsuda, Satoru; Uchida, Hiroyuki; Tsunemi, Hiroshi +1 more

We observed the southwestern region of the Cygnus Loop in two pointings with XMM-Newton. The region observed is called the "blow-out" region, which is extended further in the south. The origin of the "blow out" is not well understood, but it is suggested that there is another supernova remnant here in radio observation. To investigate in detail th…

2008 The Astrophysical Journal
XMM-Newton 20
Parallel Motions of Coronal Hard X-Ray Source and Hα Ribbons
DOI: 10.1086/592292 Bibcode: 2008ApJ...685L..87L

Gary, Dale E.; Lee, Jeongwoo

During solar flares Hα ribbons form and often move away from the local magnetic polarity inversion line (PIL). While the motion perpendicular to the PIL has been taken as evidence for coronal magnetic reconnection in the so-called CSHKP standard model, the other velocity component parallel to the PIL is much less adopted as a property of the magne…

2008 The Astrophysical Journal
SOHO 20
Photochemical Enrichment of Deuterium in Titan's Atmosphere: New Insights from Cassini-Huygens
DOI: 10.1086/595677 Bibcode: 2008ApJ...689L..61C

Mousis, Olivier; Lunine, Jonathan I.; Vuitton, Véronique +2 more

Cassini-Huygens data are used to reexamine the potential sources of the D/H enhancement over solar, measured in methane, in Titan's atmosphere. Assuming that the system is closed with respect to carbon, the use of constraints from the Huygens probe for the determination of the current mass of atmospheric methane and the most up-to-date determinati…

2008 The Astrophysical Journal
Cassini 20
Perspectives in Global Helioseismology and the Road Ahead
DOI: 10.1007/s11207-008-9136-5 Bibcode: 2008SoPh..251...53C

Chaplin, William J.; Basu, Sarbani

We review the impact of global helioseismology on key questions concerning the internal structure and dynamics of the Sun and consider the exciting challenges the field faces as it enters a fourth decade of science exploitation. We do so with an eye on the past, looking at the perspectives global helioseismology offered in its earlier phases, in p…

2008 Solar Physics
SOHO 20