Issue |
A&A
Volume 497, Number 3, April III 2009
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Page(s) | 773 - 787 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/200811471 | |
Published online | 18 February 2009 |
Online Material
Appendix A: 2-Dimensional abundances including grain surface chemistry
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Figure A.1:
Distribution of HCO+ throughout the core at four different times during the simulation for Model S. The black contour shows the outline of the disk. The disk is defined as the region where
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Figure A.2: Same as for Fig. A.1 but for N2H+. |
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Figure A.3: Same as for Fig. A.1 but for CS. |
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Figure A.4: Same as for Fig. A.1 but for SO. |
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Figure A.5: Same as for Fig. A.1 but for HCN. |
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Figure A.6: Same as for Fig. A.1 but for HNC. |
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Figure A.7: Same as for Fig. A.1 but for CN. |
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Figure A.8: Same as for Fig. A.1 but for HC3N. |
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Figure A.9: Same as for Fig. A.1 but for H2CO. |
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Figure A.10: Same as for Fig. A.1 but for CH3OH. |
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Appendix B: 2-Dimensional abundances without grain surface chemistry
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Figure B.1: Distribution of CO throughout the core at four different times during the simulation for Model G. |
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Figure B.2: Same as for Fig. B.1 but for HCO+. |
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Figure B.3: Same as for Fig. B.1 but for N2H+. |
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Figure B.4: Same as for Fig. B.1 but for CS. |
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Figure B.5: Same as for Fig. B.1 but for SO. |
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Figure B.6: Same as for Fig. B.1 but for HCN. |
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Figure B.7: Same as for Fig. B.1 but for HNC. |
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Figure B.8: Same as for Fig. B.1 but for CN. |
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Figure B.9: Same as for Fig. B.1 but for HC3N. |
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Figure B.10: Same as for Fig. B.1 but for H2CO. |
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Figure B.11: Same as for Fig. B.1 but for CH3OH. |
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