Search Publications

The nature of the molecular gas system in the core of NGC 1275
DOI: 10.1111/j.1365-2966.2005.08956.x Bibcode: 2005MNRAS.359..755W

Edge, A. C.; Johnstone, R. M.; Wilman, R. J.

We present near-infrared integral field spectroscopy of the central kiloparsec of NGC 1275 at the heart of the Perseus cluster of galaxies, obtained with the Integral Field Unit (IFU) of the United Kingdom Infrared Telescope (UKIRT) Imaging Spectrometer (UIST). The nuclear ro-vibrational H2 emission is spatially resolved and is likely t…

2005 Monthly Notices of the Royal Astronomical Society
eHST 94
Crystalline Silicates
DOI: 10.1007/s11214-005-8066-x Bibcode: 2005SSRv..119....3M

Kemper, Ciska; Molster, Frank

One of the big surprises of the Infrared Space Observatory (ISO) has been discovery of crystalline silicates outside our own Solar system. It was generally assumed before that all cosmic silicates in space were of amorphous structure. Thanks to ISO we know now that crystalline silicates are ubiquitous in the Galaxy (except for the diffuse ISM) and…

2005 Space Science Reviews
ISO 94
Energetic particle injections in Saturn's magnetosphere
DOI: 10.1029/2005GL022485 Bibcode: 2005GeoRL..3214S05M

Krupp, N.; Krimigis, S. M.; Mitchell, D. G. +9 more

Measurements from the Cassini Magnetospheric Imaging Instrument (MIMI) beginning in July 2004 reveal that sudden planetward injections of energetic ions (5-200 keV) and electrons (20-200 keV) over confined regions of azimuth are pervasive events in Saturn's magnetosphere over the radial range of 3.8 to 11.2 Saturn radii (RS). Saturn is …

2005 Geophysical Research Letters
Cassini 94
A highly-ionized absorber in the X-ray binary 4U 1323-62: A new explanation for the dipping phenomenon
DOI: 10.1051/0004-6361:20041940 Bibcode: 2005A&A...436..195B

Kaastra, J. S.; Díaz Trigo, M.; Parmar, A. N. +2 more

We report the detection of narrow Fe XXV and Fe XXVI X-ray absorption lines at 6.68 ± 0.04 keV and 6.97 ± 0.05 keV in the persistent emission of the dipping low-mass X-ray binary 4U 1323-62 during a 2003 January XMM-Newton observation. These features are superposed on a broad emission feature centered on 6.6 +0.1-0.2 keV. Dur…

2005 Astronomy and Astrophysics
XMM-Newton 94
A Chandra Study of the Multicomponent X-Ray Emission from the X-shaped Radio Galaxy 3C 403
DOI: 10.1086/427822 Bibcode: 2005ApJ...622..149K

Hardcastle, M. J.; Worrall, D. M.; Murray, S. S. +1 more

We present results from a 49.4 ks Chandra ACIS-S observation of the nearby (z=0.059) X-shaped FR type II (FR II) radio galaxy 3C 403. This is the first Chandra observation of an X-shaped radio galaxy, and one of the goals of this pioneering study is to determine the relationship between the X-ray-emitting gas and the X-shaped radio morphology. We …

2005 The Astrophysical Journal
eHST 94
The first observed stellar X-ray flare oscillation: Constraints on the flare loop length and the magnetic field
DOI: 10.1051/0004-6361:20052834 Bibcode: 2005A&A...436.1041M

Mitra-Kraev, U.; Harra, L. K.; Williams, D. R. +1 more

We present the first X-ray observation of an oscillation during a stellar flare. The flare occurred on the active M-type dwarf AT Mic and was observed with XMM-Newton. The soft X-ray light curve (0.2-12 keV) is investigated with wavelet analysis. The flare's extended, flat peak shows clear evidence for a damped oscillation with …

2005 Astronomy and Astrophysics
XMM-Newton 93
The Opacity of Spiral Galaxy Disks. IV. Radial Extinction Profiles from Counts of Distant Galaxies Seen through Foreground Disks
DOI: 10.1086/427716 Bibcode: 2005AJ....129.1396H

Allen, Ronald J.; Holwerda, B. W.; van der Kruit, P. C. +1 more

Dust extinction can be determined from the number of distant field galaxies seen through a spiral disk. To calibrate this number for the crowding and confusion introduced by the foreground image, González et al. and Holwerda et al. developed the Synthetic Field Method (SFM), which analyzes synthetic fields constructed by adding various deep exposu…

2005 The Astronomical Journal
eHST 93
Drift-Kinetic Alfvén Waves Observed near a Reconnection X Line in the Earth's Magnetopause
DOI: 10.1103/PhysRevLett.95.065002 Bibcode: 2005PhRvL..95f5002C

Balogh, A.; Reme, H.; Goldstein, M. L. +7 more

We identify drift-kinetic Alfvén waves in the vicinity of a reconnection X line on the Earth’s magnetopause. The dispersive properties of these waves have been determined using wavelet interferometric techniques applied to multipoint observations from the Cluster spacecraft. Comparison of the observed wave dispersion with that expected for drift-k…

2005 Physical Review Letters
Cluster 93
An X-Ray Variable Millisecond Pulsar in the Globular Cluster 47 Tucanae: Closing the Link to Low-Mass X-Ray Binaries
DOI: 10.1086/432249 Bibcode: 2005ApJ...630.1029B

Bogdanov, Slavko; van den Berg, Maureen; Grindlay, Jonathan E.

We report the discovery of peculiar X-ray spectral variability in the binary radio millisecond pulsar PSR J0024-7204W in the globular cluster 47 Tuc. The observed emission consists of a dominant nonthermal component, which is eclipsed for a portion of the orbit, and a thermal component, which appears to be persistent. We propose that the nontherma…

2005 The Astrophysical Journal
eHST 93
Size distribution of circumstellar disks in the Trapezium cluster
DOI: 10.1051/0004-6361:20053540 Bibcode: 2005A&A...441..195V

Alves, J.; Vicente, S. M.

In this paper we present results on the size distribution of circumstellar disks in the Trapezium cluster as measured from HST/WFPC2 data. Direct diameter measurements of a sample of 135 bright proplyds and 14 silhouettes disks suggest that there is a single population of disks well characterized by a power-law distribution with…

2005 Astronomy and Astrophysics
eHST 93