Add to ORKGThe chemical composition of cometary nuclei and the velocity field of the ejected daughter species were investigated through conventional, high-resolution spectroscopy and indirectly by imaging the dissociation radicals in the outflowing cometary comae. Gas production rates and comae symmetries were studied, and coma outflow mechanisms were modeled
We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose co...
We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose co...
The inner solar system passes of the bright comets C/1995 O1 Hale-Bopp and C/1996 B2 Hyakutake, coup...
Observations of NH2, OI, CH, CO(+), CO2(+), H2O(+), and N2(+) in optical spectra of comets represent...
Laboratory experiments are described that provide fundamental information about photochemical proces...
The composition, origins, and evolution of comets were studied. The composition was studied using sp...
Comets provide clues to the physical and chemical conditions in the early Solar System. A powerful t...
Comets provide clues to the physical and chemical conditions in the early Solar System. A powerful t...
Comets provide clues to the physical and chemical conditions in the early Solar System. A powerful t...
In order to understand the physical and chemical processes which produce the observed spatial morpho...
The objective is to investigate the spectroscopic and morphological characteristics of comets and se...
Comets are frozen remnants from the formation of the Solar System. As such, their chemical compositi...
Cometary nuclei may be our best available probes of the physical and chemical nature of the presolar...
A computer model of comet comae is described; results from assumed composition of frozen gases are s...
During 1990, a significant step was made in asertaining the molecular composition of comets by our P...
We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose co...
We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose co...
The inner solar system passes of the bright comets C/1995 O1 Hale-Bopp and C/1996 B2 Hyakutake, coup...
Observations of NH2, OI, CH, CO(+), CO2(+), H2O(+), and N2(+) in optical spectra of comets represent...
Laboratory experiments are described that provide fundamental information about photochemical proces...
The composition, origins, and evolution of comets were studied. The composition was studied using sp...
Comets provide clues to the physical and chemical conditions in the early Solar System. A powerful t...
Comets provide clues to the physical and chemical conditions in the early Solar System. A powerful t...
Comets provide clues to the physical and chemical conditions in the early Solar System. A powerful t...
In order to understand the physical and chemical processes which produce the observed spatial morpho...
The objective is to investigate the spectroscopic and morphological characteristics of comets and se...
Comets are frozen remnants from the formation of the Solar System. As such, their chemical compositi...
Cometary nuclei may be our best available probes of the physical and chemical nature of the presolar...
A computer model of comet comae is described; results from assumed composition of frozen gases are s...
During 1990, a significant step was made in asertaining the molecular composition of comets by our P...
We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose co...
We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose co...
The inner solar system passes of the bright comets C/1995 O1 Hale-Bopp and C/1996 B2 Hyakutake, coup...