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Hot Coronal Loop Oscillations Observed by SUMER: Slow Magnetosonic Wave Damping by Thermal Conduction
DOI: 10.1086/345548 Bibcode: 2002ApJ...580L..85O

Ofman, L.; Wang, Tongjiang

Recently, strongly damped Doppler shift oscillations of hot (T>6 MK) coronal loops were observed with the Solar Ultraviolet Measurement of Emitted Radiation (SUMER) spectrometer on board the Solar and Heliospheric Observatory. The oscillations are interpreted as signatures of slow-mode magnetosonic waves excited impulsively in the loops. Using …

2002 The Astrophysical Journal
SOHO 229
Solar Phenomena Associated with ``EIT Waves''
DOI: 10.1086/339402 Bibcode: 2002ApJ...569.1009B

Thompson, B. J.; Biesecker, D. A.; Vourlidas, A. +2 more

In an effort to understand what an ``EIT wave'' is and what its causes are, we have looked for correlations between the initiation of EIT waves and the occurrence of other solar phenomena. An EIT wave is a coronal disturbance, typically appearing as a diffuse brightening propagating across the Sun. A catalog of EIT waves, covering the period from …

2002 The Astrophysical Journal
SOHO 228
Measurement of Magnetic Helicity Injection and Free Energy Loading into the Solar Corona
DOI: 10.1086/342171 Bibcode: 2002ApJ...577..501K

Kusano, K.; Sakurai, T.; Yokoyama, T. +1 more

We develop a new methodology that can determine magnetic helicity flux as well as Poynting flux across the photosphere based on magnetograph observation. By applying this method, we study the injection mechanism of magnetic helicity and magnetic free energy into the solar corona. In order to derive the helicity and energy fluxes, first the velocit…

2002 The Astrophysical Journal
SOHO 228
Toward a Mass and Radius Determination of the Nearby Isolated Neutron Star RX J185635-3754
DOI: 10.1086/324296 Bibcode: 2002ApJ...564..981P

Walter, Frederick M.; Neuhäuser, Ralph; Lattimer, James M. +3 more

We discuss efforts to determine the mass, radius, and surface composition of the nearby compact object RX J185635-3754 from its multiwavelength spectral energy distribution. We compute nonmagnetized model atmospheres and emergent spectra for selected compositions and gravities and discuss efforts to fit existing and new observational data from ROS…

2002 The Astrophysical Journal
eHST 227
Large-Amplitude X-Ray Outbursts from Galactic Nuclei: A Systematic Survey using ROSAT Archival Data
DOI: 10.1086/342280 Bibcode: 2002AJ....124.1308D

Brandt, W. N.; Eracleous, Michael; Boller, Th. +1 more

In recent years, luminous X-ray outbursts with variability amplitudes as high as ~400 have been serendipitously detected from a small number of active and inactive galaxies. These outbursts may result from the tidal disruptions of stars by supermassive black holes, as well as accretion disk instabilities. In order to place the first reliable const…

2002 The Astronomical Journal
XMM-Newton 227
The Luminosity Function of Star Clusters in Spiral Galaxies
DOI: 10.1086/342381 Bibcode: 2002AJ....124.1393L

Larsen, Søren S.

Star clusters in six nearby spiral galaxies are examined using archive images from the Wide Field Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope (HST). The galaxies have previously been studied from the ground and some of them are known to possess rich populations of ``young massive clusters.'' Comparison with the HST images indica…

2002 The Astronomical Journal
eHST 227
Mid-Infrared line diagnostics of active galaxies. A spectroscopic AGN survey with ISO-SWS
DOI: 10.1051/0004-6361:20021043 Bibcode: 2002A&A...393..821S

Lutz, D.; Genzel, R.; Sturm, E. +5 more

We present medium resolution (R ~ 1500) ISO-SWS 2.4-45 mu m spectra of a sample of 29 galaxies with active nuclei. This data set is rich in fine structure emission lines tracing the narrow line regions and (circum-)nuclear star formation regions, and it provides a coherent spectroscopic reference for future extragalactic studies in the mid-infrare…

2002 Astronomy and Astrophysics
ISO 221
Coronal Holes and the High-Speed Solar Wind
DOI: 10.1023/A:1020840004535 Bibcode: 2002SSRv..101..229C

Cranmer, Steven R.

Coronal holes are the lowest density plasma components of the Sun's outer atmosphere, and are associated with rapidly expanding magnetic fields and the acceleration of the high-speed solar wind. Spectroscopic and polarimetric observations of the extended corona, coupled with interplanetary particle and radio sounding measurements going back severa…

2002 Space Science Reviews
SOHO 220
Doppler Shift Oscillations of Hot Solar Coronal Plasma Seen by SUMER: A Signature of Loop Oscillations?
DOI: 10.1086/342189 Bibcode: 2002ApJ...574L.101W

Solanki, S. K.; Curdt, W.; Innes, D. E. +2 more

We report observations of strongly damped Doppler shift oscillations detected in a flare line, Fe XIX, with the Solar Ultraviolet Measurement of Emitted Radiation spectrometer. Spectra were recorded above an active region at the western limb of the Sun, from lines with formation temperatures ranging from 0.01 to 10 MK. However, the oscillations we…

2002 The Astrophysical Journal
SOHO 219
Hubble Space Telescope and Chandra Monitoring of the Crab Synchrotron Nebula
DOI: 10.1086/344132 Bibcode: 2002ApJ...577L..49H

Gallagher, J. S.; Mori, K.; Hester, J. J. +6 more

We report the results of coordinated Hubble Space Telescope and Chandra observations of the Crab synchrotron nebula. Similar dynamical structures, including equatorial wisps moving outward at ~0.5c, are seen in both passbands. The inner X-ray ring is a variable, irregular structure from which wisps and diffuse emission emerge. The X-ray/visible je…

2002 The Astrophysical Journal
eHST 218