Search Publications

Water Production of Comets 2P/Encke and 81P/Wild 2 Derived from SWAN Observations during the 1997 Apparition
DOI: 10.1006/icar.2001.6637 Bibcode: 2001Icar..152..268M

Schmidt, W.; Bertaux, J. -L.; Lallement, R. +5 more

The water production rates of comets 2P/Encke and 81P/Wild 2 during their 1997 apparitions have been estimated from Lyman-α observations of the SWAN instrument and compared to previously published values. 2P/Encke was detected 28 times from few days preperihelion to 1.4 AU postperihelion with a perihelion water production rate QH 2

2001 Icarus
SOHO 30
A complete relativistic ionized accretion disc in Cygnus X-1
DOI: 10.1046/j.1365-8711.2001.04498.x Bibcode: 2001MNRAS.325.1045Y

Young, A. J.; Fabian, A. C.; Ross, R. R. +1 more

The galactic black hole candidate Cygnus X-1 is observed to be in one of two X-ray spectral states: either the low/hard (low soft X-ray flux and a flat power-law tail) or high/soft (high blackbody-like soft X-ray flux and a steep power-law tail) state. The physical origin of these two states is unclear. We present here a model of an ionized accret…

2001 Monthly Notices of the Royal Astronomical Society
Exosat 30
Solar cycle variations in the electron heat flux: Ulysses observations
DOI: 10.1029/2001GL012925 Bibcode: 2001GeoRL..28.2169S

Lin, Naiguo; Gary, S. Peter; Scime, Earl E. +2 more

Solar wind observations by the Ulysses spacecraft now include nearly ten years of continuous ion and electron measurements. In this study, we report detailed measurements of the electron heat flux in the solar wind. In particular, we examine the heat flux measurements for long-term correlations with wave activity and solar wind speed. We find that…

2001 Geophysical Research Letters
Ulysses 30
The Heliospheric Magnetic Field at Solar Maximum: Ulysses Observations
DOI: 10.1023/A:1011854901760 Bibcode: 2001SSRv...97..147B

Balogh, André; Smith, Edward J.

At solar maximum, the large-scale structure of the heliospheric magnetic field (HMF) reflects the complexity of the Sun's coronal magnetic fields. The corona is characterised by mostly closed magnetic structures and short-lived, small coronal holes. The axis of the Sun's dipole field is close to the solar equator; there are also important contribu…

2001 Space Science Reviews
Ulysses 30
The first XMM-Newton spectrum of a high redshift quasar - PKS 0537-286
DOI: 10.1051/0004-6361:20000423 Bibcode: 2001A&A...365L.116R

Tiengo, A.; Boller, Th.; O'Brien, P. T. +6 more

We present XMM-Newton observations of the high redshift (z=3.104), radio-loud quasar PKS 0537-286. The EPIC CCD cameras provide the highest signal-to-noise spectrum of a high-z quasar to date. The EPIC observations show that PKS 0537-286 is extremely X-ray luminous (LX =2 1047 erg s-1), with an unusually hard X-ray…

2001 Astronomy and Astrophysics
XMM-Newton 29
Circumnuclear Spiral Arms and Starburst Rings in Magnetized Barred Spiral Galaxies
DOI: 10.1086/320491 Bibcode: 2001ApJ...553L..35L

Fan, Zuhui; Lou, Yu-Qing; Yuan, Chi +1 more

The Seyfert galaxy NGC 1097 has a prominent bar and a luminous circumnuclear starburst ``ring.'' Magnetic fields as revealed by nonthermal radio continuum emissions correlate well with the optical barred spiral structure on large scales, have a gross enhancement overlapping with the optical/infrared ``ring,'' and show a trailing swirl around and w…

2001 The Astrophysical Journal
eHST 29
The Massive Star Content of NGC 6822: Ground-Based andHubble Space Telescope Photometry
DOI: 10.1086/319969 Bibcode: 2001AJ....121.2020B

Massey, Philip; Bianchi, Luciana; Romaniello, Martino +1 more

We investigate the massive star population of NGC 6822 with ground-based UBV photometry covering the whole of the galaxy and HST WFPC2 photometry with filters F255W, F336W, F439W, and F555W of two fields containing very rich and crowded OB associations. The four-band WFPC2 photometry is used to derive Teff and E(B-V). H-R diagrams are c…

2001 The Astronomical Journal
eHST 29
Gas-Phase Polycyclic Aromatic Hydrocarbons in Absorption toward Protostellar Sources?
DOI: 10.1086/321347 Bibcode: 2001ApJ...554..126B

Bregman, Jesse D.; Temi, Pasquale

One of the major criticisms of identifying the infrared emission bands with polycyclic aromatic hydrocarbon (PAH) molecules has been the lack of a match between laboratory spectra of individual PAHs and the emission features. Part of the difficulty arises from the complexity of modeling the emission mechanism with an a priori unknown mixture of io…

2001 The Astrophysical Journal
ISO 29
Four years of Ulysses dust data: 1996-1999
DOI: 10.1016/S0032-0633(01)00054-X Bibcode: 2001P&SS...49.1303K

Krüger, H.; Srama, R.; Hamilton, D. P. +17 more

The Ulysses spacecraft is orbiting the Sun on a highly inclined ellipse ( i=79°, perihelion distance 1.3 AU, aphelion distance 5.4 AU). Between January 1996 and December 1999 the spacecraft was beyond 3 AU from the Sun and crossed the ecliptic plane at aphelion in May 1998. In this 4-yr period 218 dust impacts were recorded with the dust detector …

2001 Planetary and Space Science
Ulysses 29
Possible contribution of different energy sources to the production of organics in Titan's atmosphere
DOI: 10.1016/S0273-1177(01)00056-4 Bibcode: 2001AdSpR..27..261R

Coll, P.; Raulin, F.; Navarro-González, R. +1 more

A quantitative comparison of the products arising from the irradiation of a Titan's simulated atmosphere is presented. The energy sources used represent some of the main events that occur in the satellite's atmosphere. All of the compounds identified are classified in the hydrocarbon and nitrile chemical families. Almost all of the detected compou…

2001 Advances in Space Research
Huygens 29