Search Publications

Chemical composition of Titan's haze: Are PAHs present?
DOI: 10.1029/2004GL019859 Bibcode: 2004GeoRL..3117S08T

McKay, Christopher P.; Toon, Owen B.; Trainer, Melissa G. +4 more

Previous laboratory studies of haze aerosols analogous to those in Titan's atmosphere have shown evidence of the formation of polycyclic aromatic hydrocarbons (PAHs). If present, PAHs may provide a mechanism for both particle formation and nitrogen incorporation. We have conducted new experiments simulating Titan haze production using an Aerosol M…

2004 Geophysical Research Letters
Huygens 25
Kinematics of stellar associations: the epicycle approximation and the convergent point method
DOI: 10.1111/j.1365-2966.2004.08012.x Bibcode: 2004MNRAS.352.1199M

Olling, Rob P.; Makarov, Valeri V.; Teuben, Peter J.

Employing analytical and numerical tools, we expound the Galactic epicycle theory to describe the kinematic evolution of stellar, gravitationally unbound associations in the vicinity of the Sun. We estimate the limits of applicability of the analytical epicycle approximation and harmonic vertical motion by numerical integration of test orbits with…

2004 Monthly Notices of the Royal Astronomical Society
Hipparcos 25
High resolution millimeter imaging of the proto-planetary nebula He 3-1475
DOI: 10.1051/0004-6361:20034139 Bibcode: 2004A&A...414..581H

Bachiller, R.; Forveille, T.; Cox, P. +2 more

We report high resolution (1 arcsec-2 arcsec) imaging of the CO 2-1 line and the millimeter continuum in the proto-planetary nebula He 3-1475. The observations reveal the presence of a massive (∼ 0.6 M) envelope of molecular gas around the origin of the remarkable bipolar jet system seen in optical images with the HST. The CO kinematic…

2004 Astronomy and Astrophysics
eHST 24
Orientation and motion of a discontinuity from single-spacecraft measurements of plasma velocity and density: Minimum mass flux residue
DOI: 10.1029/2003JA010230 Bibcode: 2004JGRA..109.3221S

Balogh, A.; Lavraud, B.; Dunlop, M. W. +4 more

A simple analytical solution is presented to the problem of determining the orientation and motion of a one-dimensional discontinuity in plasma velocity and density, measured by a single spacecraft as the discontinuity moves past it. The method developed is called Minimum Massflux Residue (MMR). Illustrations of the method, based on Cluster measur…

2004 Journal of Geophysical Research (Space Physics)
Cluster 24
Time-dependent ejection velocity model for the outflow of Hen 3-1475
DOI: 10.1051/0004-6361:20035757 Bibcode: 2004A&A...419..991V

Velázquez, P. F.; Raga, A. C.; Riera, A.

We present 2D axisymmetric and 3D numerical simulations of the proto-planetary nebula Hen 3-1475, which is characterized by a remarkably highly collimated optical jet, formed by a string of shock-excited knots along the axis of the nebula. It has recently been suggested that the kinematical and morphological properties of the

2004 Astronomy and Astrophysics
eHST 24
Impulsive and Gradual Nonthermal Emissions in an X-Class Flare
DOI: 10.1086/381353 Bibcode: 2004ApJ...603..335Q

Qiu, Jiong; Gary, Dale E.; Lee, Jeongwoo

In this paper we present a comprehensive case study of an X-class flare observed on 2001 April 6. The flare consists of two episodes, the first characterized by impulsive spiky bursts and the second by gradual smooth emission at hard X-ray and microwave wavelengths. Emissions in the two episodes are regarded as the impulsive and gradual components…

2004 The Astrophysical Journal
SOHO 24
Ulysses Observations of the Magnetic Connectivity between Coronal Mass Ejections and the Sun
DOI: 10.1086/420811 Bibcode: 2004ApJ...608.1100R

Crooker, N. U.; Riley, Pete; Gosling, J. T.

We have investigated the magnetic connectivity of coronal mass ejections (CMEs) to the Sun using Ulysses observations of suprathermal electrons at various distances between 1 and 5.2 AU. Drawing on ideas concerning the eruption and evolution of CMEs, we had anticipated that there might be a tendency for CMEs to contain progressively more open fiel…

2004 The Astrophysical Journal
Ulysses 24
XMM-Newton Spectroscopy of Four Bright Ultraluminous X-Ray Sources in the Antennae Galaxies (NGC 4038/4039)
DOI: 10.1086/421098 Bibcode: 2004ApJ...609..728M

Zezas, A.; Miller, J. M.; Fabbiano, G. +1 more

We report the results of spectral fits to four bright ultraluminous X-ray sources (ULXs) in the Antennae galaxies (NGC 4038/4039) observed for 41 ks with XMM-Newton. Although emission regions are not resolved as well as in prior Chandra observations, at least four ULXs (X-11, X-16, X-37, and X-44 in the Zezas and Fabbiano scheme) are sufficiently …

2004 The Astrophysical Journal
XMM-Newton 24
Astrometric Discovery of GJ 164B
DOI: 10.1086/425653 Bibcode: 2004ApJ...617.1323P

Henry, Todd; Benedict, G. Fritz; Pravdo, Steven H. +1 more

We discovered a low-mass companion to the M dwarf GJ 164 with the CCD-based imaging system of the Stellar Planet Survey astrometric program. The existence of GJ 164B was confirmed with Hubble Space Telescope NICMOS imaging observations. A high-dispersion spectral observation in V sets a lower limit of Δm>2.2 mag between the two components of th…

2004 The Astrophysical Journal
eHST 24
12C/13C Ratio in Planetary Nebulae from the IUE Archives
DOI: 10.1086/382528 Bibcode: 2004ApJ...605..784R

Ferland, G. J.; Rubin, R. H.; Chollet, E. E. +1 more

We investigated the abundance ratio of 12C/13C in planetary nebulae by examining emission lines arising from C III 2s2p3Po2,1,0-->2s21S0. Spectra were retrieved from the International Ultraviolet Explorer archives, and multiple spectra of the same object wer…

2004 The Astrophysical Journal
IUE 24