Search Publications

Densities and Velocities in Fast Coronal Mass Ejections: Radiative Pumping of the O VI Doublet
DOI: 10.1086/421391 Bibcode: 2004ApJ...606L.159R

Raymond, J. C.; Ciaravella, A.

In very fast coronal mass ejections (CMEs), it is possible for O VI ions to scatter Lyβ photons that originate in the solar chromosphere and for the λ1037 transition of O VI to scatter λ1032 photons from the solar transition region. This scattering process can be identified by departures of the O VI I1032/I1037 intensity rati…

2004 The Astrophysical Journal
SOHO 23
Very High Iron Abundance of the Hot Gas around the cD Galaxy of the MKW 4 Cluster
DOI: 10.1086/421345 Bibcode: 2004ApJ...606L.109F

Fukazawa, Yasushi; Kawano, Naomi; Kawashima, Kengo

We observed a nearby X-ray-bright poor cluster MKW 4 with Chandra. The iron abundance is found to increase dramatically from 0.3 to 1.3 solar within 150" of the cD galaxy NGC 4073. Then MKW 4 is the second cluster to exhibit a significantly high metallicity of greater than 1 solar, after the Centaurus Cluster. Weakness of the central cool componen…

2004 The Astrophysical Journal
XMM-Newton 23
A View of PKS 2155-304 with XMM-Newton Reflection Grating Spectrometers
DOI: 10.1086/381698 Bibcode: 2004ApJ...603..449C

Maraschi, L.; Tavecchio, F.; Treves, A. +2 more

We present the high-resolution X-ray spectrum of the BL Lac object PKS 2155-304 taken with the RGS units on board XMM-Newton in 2000 November. We detect an O VII Kα resonant absorption line from warm/hot local gas at 21.59 Å (~4.5 σ detection). The line profile is possibly double peaked. We do not confirm the strong 20.02 Å absorption line seen wi…

2004 The Astrophysical Journal
XMM-Newton 23
Pickup ions at Dione and Enceladus: Cassini Plasma Spectrometer simulations
DOI: 10.1029/2002JA009647 Bibcode: 2004JGRA..109.1214S

Crary, F.; Johnson, R. E.; Young, D. T. +5 more

Voyager images of the icy satellites of Saturn, Dione and Enceladus, suggest that they may have been geologically active and are not only composed of ice. Recent observations by the Hubble Space Telescope have shown the presence of ozone at both Dione and Rhea, which also implies the presence of molecular oxygen at these bodies. Observations of Ar…

2004 Journal of Geophysical Research (Space Physics)
Cassini 23
Flow burst-induced large-scale plasma sheet oscillation
DOI: 10.1029/2004JA010533 Bibcode: 2004JGRA..10911208V

Balogh, A.; Glassmeier, K. -H.; RèMe, H. +7 more

On 12 August 2001 the Cluster spacecraft measured a rapid flux transport event, consisting of a strong perpendicular earthward flow burst combined with a dipolarization of the magnetic field after a strong compression of the magnetotail. Combining the Cluster data with those from ground-based magnetometers, we find that this event is related to pa…

2004 Journal of Geophysical Research (Space Physics)
Cluster 23
Looking Closely at Medusa: Star-forming Knots at the Center of NGC 4194
DOI: 10.1086/382092 Bibcode: 2004AJ....127.1360W

Kaiser, M. E.; Weistrop, D.; Eggers, D. +3 more

We report high-resolution ultraviolet and visible-wavelength imaging of the blue compact galaxy NGC 4194 (the Medusa) using the Hubble Space Telescope. A complete sample of 38 UV-bright knots is identified. These knots produce 20% of the ultraviolet emission from the area of the galaxy observed. The bright end of the knot flux distribution can be …

2004 The Astronomical Journal
eHST 22
Boron Benchmarks for the Galactic Disk
DOI: 10.1086/382672 Bibcode: 2004ApJ...606..306B

Cunha, Katia; McGrath, Elizabeth J.; Lambert, David L. +1 more

Sixteen Population I solar-type dwarfs have been selected to ascertain the baseline B abundance in the Galactic disk for a range of a factor of 4 in metallicity: from [Fe/H] of -0.5 to +0.1. All the stars selected are undepleted in Be, which ensures that they have also retained their full initial abundance of B. Evaluation of the trend of B with F…

2004 The Astrophysical Journal
eHST 22
XMM-Newton observations of the young open cluster Blanco 1. I. X-ray spectroscopy and photometry
DOI: 10.1051/0004-6361:20035869 Bibcode: 2004A&A...421..175P

Harnden, F. R., Jr.; Micela, G.; Sciortino, S. +2 more

We present an X-ray study of the high metallicity young open cluster Blanco 1 based on XMM-Newton data. X-ray spectroscopy of cluster members is presented for the first time as well as new X-ray distribution functions of late-type stars. We detected all known dF and dG stars in the EPIC field and 80% and 90% of dK and dM stars, respectively. The X…

2004 Astronomy and Astrophysics
XMM-Newton 22
On the propagation of low-frequency fluctuations in the plasma sheet: 1. Cluster observations and magnetohydrodynamic analysis
DOI: 10.1029/2003JA010228 Bibcode: 2004JGRA..109.3216L

Budnik, E.; Balogh, A.; Lucek, E. +6 more

Low-frequency pressure and magnetic oscillations observed by Cluster in the plasma sheet are investigated with the aim of determining if they are magnetohydrodynamic (MHD) eigenmodes. We analyze the plasma sheet crossing occurring on 22 August 2001, as the magnetosphere was first quiet and then active, and compare the observations with theoretical…

2004 Journal of Geophysical Research (Space Physics)
Cluster 22
On the propagation of low-frequency fluctuations in the plasma sheet: 2. Characterization of the MHD eigenmodes and physical implications
DOI: 10.1029/2003JA010229 Bibcode: 2004JGRA..109.3217F

Budnik, E.; Balogh, A.; Lucek, E. +7 more

In a first analysis of the low-frequency fluctuations observed by Cluster during a crossing of the plasma sheet [, 2004], we identify oscillations that likely correspond to MHD eigenmodes. They are intense (10 nT), have a rather short period (20-25 s), have a wavelength of ∼5 Re, and are observed during an active period that follows a s…

2004 Journal of Geophysical Research (Space Physics)
Cluster 22