Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



  history
ID: 225870.0, MPI für Astronomie / Publikationen_mpia
Ionization structure of protoplanetary disks from the chemical perspective
Authors:Wiebe, D.; Semenov, D.; Henning, Th.
Date of Publication (YYYY-MM-DD):2004
Title of Journal:Baltic Astronomy
Volume:13
Start Page:459
End Page:463
Review Status:not specified
Audience:Not Specified
Abstract / Description:We review the major chemical processes,
responsible for the fractional ionization in a
typical protoplanetary disk and indicate the
possibility to reduce the number of species and
reactions in a chemical model that might be used
to compute the ionization degree in these objects.
Free Keywords:astrochemistry; stars: formation; molecular
; processes; ISM: molecules; ISM: abundances
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
External Affiliations:Moscow 119017, Russia), AB(Astrophysical
Institute and University Observatory,
Schillerg‚‚auml;‚‚szlig;chen 2-3, D-07745 Jena,
Germany), AC(Max-Planck-Institut f‚‚uuml;r
Astronomie, K‚‚ouml;nigstuhl 17, D-69117
Heidelberg, Germany)
Identifiers:URL:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bi... [ID No:1]
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.