J/A+A/535/A117ivo://CDS.VizieR/J/A+A/535/A117doi:10.26093/cds/vizier.35350117CDSSterling N.C.Stancil P.C.2017-10-09T13:33:35Z2011-11-22T08:23:06ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fratomic-physicsWe present total and final-state resolved charge transfer (CT) rate coefficients for low-charge Ge, Se, Br, Kr, Rb, and Xe ions reacting with neutral hydrogen over the temperature range 102-106K. Each of these elements has been detected in ionized astrophysical nebulae, particularly planetary nebulae. CT rate coefficients are a key ingredient for the ionization equilibrium solutions needed to determine total elemental abundances from those of the observed ions. A multi-channel Landau Zener approach was used to compute rate coefficients for projectile ions with charges q=2-5, and for singly-charged ions the Demkov approximation was utilized.2011A&A...535A.117Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/535/A117CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/529/A147 : Selenium ions photoionization cross sections (Sterling+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/535/A117https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/535/A117http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/535/A117https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/535/A117https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/535/A117http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/535/A117GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/535/A117/ratesFinal-state resolved charge transfer recombination rate coefficients (cm^3^/s) for the reactions X^q+^+H --> X^(q-1)+^+H^+^+{delta}E (table4) and X^0^+H^+^ --> X^+^+H+{delta}E (table5)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElProjectile element (Ge Se Br Kr Rb Xe)phys.atmol.elementcharion[0/5] Ionisation statephys.atmol.ionStageintTarSimbad column added by the CDSphys.atmol.elementcharExitCExit channelphys.atmol.configurationa(0.1)Rate coefficient {alpha} over T=100K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(0.2)Rate coefficient {alpha} over T=200K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(0.4)Rate coefficient {alpha} over T=400K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(0.6)Rate coefficient {alpha} over T=600K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(0.8)Rate coefficient {alpha} over T=800K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(1.0)Rate coefficient {alpha} over T=1000K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(1.2)Rate coefficient {alpha} over T=2000K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(1.4)Rate coefficient {alpha} over T=4000K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(1.6)Rate coefficient {alpha} over T=6000K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(1.8)Rate coefficient {alpha} over T=8000K (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(10.)Rate coefficient {alpha} over T=10kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(20.)Rate coefficient {alpha} over T=20kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(40.)Rate coefficient {alpha} over T=40kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(60.)Rate coefficient {alpha} over T=60kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(80.)Rate coefficient {alpha} over T=80kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(100)Rate coefficient {alpha} over T=100kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(200)Rate coefficient {alpha} over T=200kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(400)Rate coefficient {alpha} over T=400kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(600)Rate coefficient {alpha} over T=600kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdoublea(800)Rate coefficient {alpha} over T=800kK (1)cm**3.s**-1arith.rate;phys.atmol.transProbdouble