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ISO LWS Observations of the Two Nearby Spiral Galaxies NGC 6946 and NGC 1313
DOI: 10.1086/341374 Bibcode: 2002AJ....124..751C

Dale, Daniel A.; Rubio, Monica; Rubin, Robert H. +8 more

We present the analysis of Infrared Space Observatory long-wavelength spectrometer (LWS) observations of the two nearby late-type galaxies NGC 1313 and NGC 6946. Both galaxies have been fully mapped in the [C II] far-infrared fine-structure line at 158 µm, and some regions have been observed also in the [O I] 63 µm and [N II] 122 &micr…

2002 The Astronomical Journal
ISO 43
Hubble Space Telescope/NICMOS Observations of Terzan 5: Stellar Content and Structure of the Core
DOI: 10.1086/339874 Bibcode: 2002ApJ...571..818C

Cohn, Haldan N.; Lugger, Phyllis M.; Edmonds, Peter D. +1 more

We report results from Hubble Space Telescope/NICMOS imaging of the extremely dense core of the globular cluster Terzan 5. This highly obscured bulge cluster contains a low-mass X-ray binary and at least two millisecond pulsars, with evidence for a large millisecond pulsar population. It has been estimated to have one of the highest collision rate…

2002 The Astrophysical Journal
eHST 43
X-Ray Bright Points and Photospheric Bipoles during Cycles 22 and 23
DOI: 10.1086/324306 Bibcode: 2002ApJ...564.1042S

Pevtsov, Alexei A.; Sattarov, Isroil; Hojaev, Alisher S. +1 more

We use the Yohkoh soft X-ray telescope (SXT) full-disk images made from 1993 to 2000 to manually identify X-ray bright points (XBPs). We also employ the National Solar Observatory (Kitt Peak) full-disk longitudinal magnetograms made between 1992 April and 2001 April and an automatic procedure to identify photospheric bipoles whose magnetic field s…

2002 The Astrophysical Journal
SOHO 43
Organic Chemistry and Exobiology on Titan
DOI: 10.1023/A:1023636623006 Bibcode: 2002SSRv..104..377R

Owen, Tobias; Raulin, François

Exobiology is not only the study of the origin, distribution and evolution of life in the universe, but also of structures — including at the molecular level, and processes — including organic chemical transformations — related to life. In that respect, with its dense nitrogen atmosphere, which includes a noticeable fraction of methane, and the ma…

2002 Space Science Reviews
Huygens 42
Thermal Pressures in Neutral Clouds inside the Local Bubble, as Determined from C I Fine-Structure Excitations
DOI: 10.1086/343796 Bibcode: 2002ApJ...580..938J

Jenkins, Edward B.

High-resolution spectra covering the absorption features from interstellar C I were recorded for four early-type stars with spectrographs on the Hubble Space Telescope, in a program to measure the fine-structure excitation of this atom within neutral clouds inside or near the edge of the Local Bubble, a volume of hot (T~106K) gas that e…

2002 The Astrophysical Journal
eHST 42
Cluster observations of fast magnetosonic waves in the terrestrial foreshock
DOI: 10.1029/2002GL015582 Bibcode: 2002GeoRL..29.2046E

Balogh, A.; Dandouras, I.; Eastwood, J. P. +2 more

Cluster observations of ULF waves in the terrestrial foreshock are presented. Four spacecraft timing techniques on magnetic field measurements are used with plasma bulk velocity measurements to determine wave properties in the plasma rest frame. Based on the propagation speed and polarisation, the waves are found to be fast magnetosonic. The analy…

2002 Geophysical Research Letters
Cluster 42
Magnetospheric and Plasma Science with Cassini-Huygens
DOI: 10.1023/A:1023605110711 Bibcode: 2002SSRv..104..253B

Gurnett, D. A.; Dougherty, M. K.; Tsurutani, B. T. +27 more

Magnetospheric and plasma science studies at Saturn offer a unique opportunity to explore in-depth two types of magnetospheres. These are an ‘induced’ magnetosphere generated by the interaction of Titan with the surrounding plasma flow and Saturn's ‘intrinsic’ magnetosphere, the magnetic cavity Saturn's planetary magnetic field creates inside the …

2002 Space Science Reviews
Cassini 42
The underlying direction of the heliospheric magnetic field through the Ulysses first orbit
DOI: 10.1029/2001JA005056 Bibcode: 2002JGRA..107.1405F

Balogh, A.; Forsyth, R. J.; Smith, E. J.

Between February 1992 and April 1998 the Ulysses spacecraft carried out the first survey of how the properties of the solar wind and heliospheric magnetic field vary with latitude during the declining and minimum phases of the solar cycle. In this paper we report on how the underlying direction of the heliospheric magnetic field varied through the…

2002 Journal of Geophysical Research (Space Physics)
Ulysses 42
Extragalactic globular clusters in the near infrared. I. A comparison between M87 and NGC 4478
DOI: 10.1051/0004-6361:20020831 Bibcode: 2002A&A...391..441K

Minniti, D.; Kissler-Patig, M.; Brodie, J. P.

We compare optical and near infrared colours of globular clusters in M87, the central giant elliptical in Virgo, and NGC 4478, an intermediate luminosity galaxy in Virgo, close in projection to M87. Combining V and I photometry obtained with the WFPC2 on HST and K_s photometry obtained with the NIRC on Keck 1, we find the broad range in colour and…

2002 Astronomy and Astrophysics
eHST 42
The young intermediate-mass stellar object AFGL 490 - A disk surrounded by a cold envelope
DOI: 10.1051/0004-6361:20021160 Bibcode: 2002A&A...394..561S

Henning, Th.; van Dishoeck, E. F.; van der Tak, F. F. S. +2 more

AFGL 490 is a key target of the class of deeply embedded intermediate-mass young stellar objects in a transition stage to Herbig Be stars (L = 2.2-4.0 x 103 Lsun ). In this paper, we present a comprehensive set of single-dish line data which characterize the envelope of the source. In addition, observations of CS J = 2->1 …

2002 Astronomy and Astrophysics
ISO 42