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20032011
most citedThe hydrodynamical relevance of the Camassa-Holm and Degasperis-Procesi equations

1k citations

Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA201152 cited

The end of star formation in Chamaeleon I ? A LABOCA census of starless and protostellar cores

A. Belloche, F. Schuller, B. Parise +7

Chamaeleon I is the most active region in terms of star formation in the Chamaeleon molecular cloud complex. Its population of prestellar and protostellar cores is not known and a…

astro-ph.GA201018 cited

Statistical universal branching ratios for cosmic ray dissociation, photodissociation, and dissociative recombination of the C(n=2-10), C(n=2-4)H and C3H2 neutral and cationic species

M. Chabot, T. Tuna, K. Beroff +9

Fragmentation branching ratios of electronically excited molecular species are of first importance for the modeling of gas phase interstellar chemistry. Despite experimental and th…

astro-ph.GA2010338 cited

Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT

LAT Collaboration

Pulsars are rapidly-rotating, highly-magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until r…

astro-ph.GA201016 cited

Herschel/HIFI observations of spectrally resolved methylidyne signatures toward the high-mass star-forming core NGC6334I

M. H. D. van der Wiel, F. F. S. van der Tak, D. C. Lis +65

In contrast to extensively studied dense star-forming cores, little is known about diffuse gas surrounding star-forming regions. We study molecular gas in the high-mass star-formin…

astro-ph.GA201033 cited

Kinematic parameters and membership probabilities of open clusters in the Bordeaux PM2000 catalogue

A. Krone-Martins, C. Soubiran, C. Ducourant +2

We derive lists of proper-motions and kinematic membership probabilities for 49 open clusters and possible open clusters in the zone of the Bordeaux PM2000 proper motion catalogue…

astro-ph.GA201072 cited

Sensitivity analyses of dense cloud chemical models

V. Wakelam, E. Herbst, J. Le Bourlot +3

Because of new telescopes that will dramatically improve our knowledge of the interstellar medium, chemical models will have to be used to simulate the chemistry of many regions wi…