Compolation of interstellar lines
| dc.contributor.author | Preethi, K. | |
| dc.contributor.author | Gudennavar, S. B. | |
| dc.contributor.author | Bubbly, S. G. | |
| dc.contributor.author | et al. | |
| dc.date.accessioned | 2012-03-05T09:43:51Z | |
| dc.date.available | 2012-03-05T09:43:51Z | |
| dc.date.issued | 2011-11-22 | |
| dc.description.abstract | We have collated absorption line data toward 3014 stars (Fig. 1) in order to create a unified database of interstellar column densities. These data have been taken from a number of different published sources and include many different species and ionizations. The preliminary results from our analysis show a tight relation between N(H) and E(B-V) i.e. [N(H)/E(B-V)=6.12x10²¹]. Similar plots have been obtained with many different species, and their correlations along with the correlation coefficients are presented. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/433 | |
| dc.language.iso | en | en_US |
| dc.relation.ispartofseries | International conference on Interstellar dust, molecules and chemistry (IDMC-2011), 22-25 Nov., 2011 IUCAA, Pune, India; | |
| dc.subject | Interstellar | en_US |
| dc.subject | Compilation | en_US |
| dc.subject | Posters | en_US |
| dc.title | Compolation of interstellar lines | en_US |
| dc.type | Presentation | en_US |