PHOSPHORUS CHEMISTRY IN THE SHOCKED REGION L1157 B1
Creators
- 1. Department of Earth and Planetary Sciences, Kobe University, Kobe 657-8501 (Japan)
Description
We study the evolution of phosphorus-bearing species in one-dimensional C-shock models. We find that the abundances of P-bearing species depend sensitively on the elemental abundance of P in the gas phase and on the abundance of N atoms in the pre-shock gas. The observed abundance of PN and the non-detection of PO toward L1157 B1 are reproduced in C-shock models with shock velocity v = 20 km s–1 and pre-shock density n(H2) 104-105 cm–3, if the elemental abundance of P in the gas phase is ∼10–9 and the N-atom abundance is n(N)/nH ∼10–5 in the pre-shock gas. We also find that P-chemistry is sensitive to O- and N-chemistry because N atoms are destroyed mainly by OH and NO. We identify the reactions of O-bearing and N-bearing species that significantly affect P-chemistry.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-637X/761/1/74Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 761
- Journal Issue
- 1
- Journal Page Range
- [10 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44094576
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTRONOMY; ASTROPHYSICS; ATOMS; CHEMISTRY; COSMIC GASES; ELEMENT ABUNDANCE; HYDROGEN; MOLECULES; NITRIC OXIDE; ONE-DIMENSIONAL CALCULATIONS; PHOSPHORUS; SHOCK WAVES; VELOCITY
- Descriptors DEC
- ABUNDANCE; CHALCOGENIDES; ELEMENTS; FLUIDS; GASES; NITROGEN COMPOUNDS; NITROGEN OXIDES; NONMETALS; OXIDES; OXYGEN COMPOUNDS; PHYSICS