Zobrazeno 1 - 10
of 187
pro vyhledávání: '"R. Ruiterkamp"'
Publikováno v:
Fullerenes, Nanotubes and Carbon Nanostructures. 19:398-409
We present for the first time the UV/Vis spectrum of the neutral and ionized fullerene C84 isolated in a neon matrix at low temperature. After ionization with high energy (10.2 eV) UV photons, we are able to identify a new spectroscopic absorption ba
Autor:
S. D. Rodgers, H. C. Huang, Harold M. Butner, Pascale Ehrenfreund, S. B. Charnley, R. Ruiterkamp, Yi-Jehng Kuan
Publikováno v:
Astrophysics and Space Science. 310:181-188
We have observed emission from both ortho and para spin states of ketene (CH2CO) towards several deeply-embedded protostars. The low CH2CO fractional abundances (∼10−10) and the rotation temperatures (∼20 K) are consistent with emission from th
Publikováno v:
Planetary and Space Science. 55:383-400
We studied the stability of aromatic compounds in low Earth orbit environment and describe the scientific results and successful flight of the ORGANICS experiment on-board the BIOPAN V space exposure facility. This experiment investigated the photo s
PAH charge state distribution and DIB carriers: Implications from the line of sight toward HD 147889
Autor:
Marco Spaans, L. Kaper, R. Ruiterkamp, Bernard Foing, N. L. J. Cox, Pascale Ehrenfreund, Farid Salama
Publikováno v:
Astronomy and Astrophysics
Astronomy & astrophysics, 432(2), 515-529.e9. EDP Sciences
Astronomy and Astrophysics, 432, 515-529. EDP Sciences
Astronomy & astrophysics, 432(2), 515-529.e9. EDP Sciences
Astronomy and Astrophysics, 432, 515-529. EDP Sciences
We have computed physical parameters such as density, degree of ionization and temperature, constrained by a large observational data set on atomic and molecular species, for the line of sight toward the single cloud HD147889. Diffuse interstellar ba
Autor:
Steven B. Charnley, R. Ruiterkamp, Pascale Ehrenfreund, A. J. Markwick, S. D. Rodgers, Harold M. Butner, Adwin Boogert, Tom J. Millar
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 347, 157-162. Oxford University Press
We propose a series of detailed observations that should allow current ideas concerning the important catalytic pathways to interstellar molecules on interstellar dust grains to be tested. The atoms and molecules that accrete on cold grains and take
Publikováno v:
The Astrophysical Journal. 593:L129-L132
Nucleobases are nitrogen heterocycles (N-heterocycles) that are essential components of the genetic material in all living organisms. Extraterrestrial nucleobases have been found in several carbonaceous chondrites, but only in traces. No astronomical
Autor:
Farid Salama, Martin Head-Gordon, Jennifer L. Weisman, R. Ruiterkamp, Thomas M. Halasinski, Timothy J. Lee
Publikováno v:
The Journal of Physical Chemistry A. 107:3660-3669
We present a full experimental and theoretical study of an interesting series of polycyclic aromatic hydrocarbons, the oligorylenes. The absorption spectra of perylene, terrylene and quaterrylene in neutral, cationic and anionic charge states are obt
Autor:
Bernard Foing, Pascale Ehrenfreund, Farid Salama, W. Schmidt, Louis J. Allamandola, Thomas M. Halasinski, R. Ruiterkamp
Publikováno v:
Astronomy and Astrophysics
Astronomy and Astrophysics, 390, 1153-1170. EDP Sciences
Scopus-Elsevier
Astronomy and Astrophysics, 390, 1153-1170. EDP Sciences
Scopus-Elsevier
Polycyclic Aromatic Hydrocarbons (PAHs) are thought to be the carriers of the ubiquitous infrared emission bands (UIBs). Data from the Infrared Space Observatory (ISO) have provided new insights into the size distribution and the structure of interst
Publikováno v:
Journal of Geophysical Research: Planets. 106:33291-33301
Our current knowledge on the chemical composition of interstellar ices is summarized with respect to the possible contribution of energetic photons and particles to their observed state. We describe the inventory of astronomical ices as determined by
Publikováno v:
Astronomy & Astrophysics. 367:347-354
Experiments simulating the processing of various hydrocarbon species under diffuse and dense cloud conditions by UV irradiation were performed. The results indicate that such molecules will be efficiently dehydrogenated in interstellar space. It is a