dc.contributor.author |
Roy, Arijit |
|
dc.contributor.author |
Singh, Surendra Vikram |
|
dc.contributor.author |
Meka, J. K. |
|
dc.contributor.author |
Ramachandran, R. |
|
dc.contributor.author |
Sahu, D. |
|
dc.contributor.author |
Gautam, Abhay Raj Singh |
|
dc.contributor.author |
Thiruvenkatam, Vijay |
|
dc.contributor.author |
Jayaram, V. |
|
dc.contributor.author |
Janardhan, P. |
|
dc.contributor.author |
Rajasekhar, B. N. |
|
dc.contributor.author |
Bhardwaj, Anil |
|
dc.contributor.author |
Mason, N. J. |
|
dc.contributor.author |
Sivaraman, B. |
|
dc.coverage.spatial |
United Kingdom |
|
dc.date.accessioned |
2022-10-04T12:56:38Z |
|
dc.date.available |
2022-10-04T12:56:38Z |
|
dc.date.issued |
2022-12 |
|
dc.identifier.citation |
Roy, Arijit; Singh, Surendra Vikram; Meka, J. K.; Ramachandran, R.; Sahu, D.; Gautam, Abhay Raj Singh; Thiruvenkatam, Vijay; Jayaram, V.; Janardhan, P.; Rajasekhar, B. N.; Bhardwaj, Anil; Mason, N. J. and Sivaraman, B., “Shock induced transformation of non-magnetic to magnetic ISM dust analogue”, Monthly Notices of the Royal Astronomical Society, DOI: 10.1093/mnras/stac2637, vol. 517, no. 4, pp. 4845-4855, Dec. 2022. |
en_US |
dc.identifier.issn |
0035-8711 |
|
dc.identifier.issn |
1365-2966 |
|
dc.identifier.uri |
https://doi.org/10.1093/mnras/stac2637 |
|
dc.identifier.uri |
https://repository.iitgn.ac.in/handle/123456789/8173 |
|
dc.description.abstract |
The fate of organometallic dust subjected to extreme conditions, especially the shock fronts, in the ISM has not been explored to date. Iron and cyclopentadiene, which have been found to be present in the ISM, are known to react and produce organometallic compound ferrocene under terrestrial conditions. In our experiment we subjected ferrocene, a possible proxy of such dust, to ∼ 5.6 M shock commensurate with conditions encountered in the ISM, leading to a temperature rise up to 7300 K within 2 ms. Analysis of the post-shock residue showed the presence of a α-Fe and Fe3C composite, that responded to an external magnetic field. These results show that a non-magnetic dust composed of molecules containing transition metals undergoing shock processing in the ISM can dissociate and synthesize dust that is then magnetic. Such drastic transformations from non-magnetic to magnetic dust induced by shocks might be of importance in interstellar polarization. |
|
dc.description.statementofresponsibility |
by Arijit Roy, Surendra Vikram Singh, J. K. Meka, R. Ramachandran, D. Sahu, Abhay Raj Singh Gautam, Vijay Thiruvenkatam, V. Jayaram, P. Janardhan, B. N. Rajasekhar, Anil Bhardwaj, N. J. Mason and B. Sivaraman |
|
dc.format.extent |
vol. 517, no. 4, pp. 4845-4855 |
|
dc.language.iso |
en_US |
en_US |
dc.publisher |
Royal Astronomical Society |
en_US |
dc.subject |
Shock induced transformation |
en_US |
dc.subject |
Organometallic dust |
en_US |
dc.subject |
ISM |
en_US |
dc.subject |
Interstellar polarization |
en_US |
dc.subject |
Magnetic dust |
en_US |
dc.title |
Shock induced transformation of non-magnetic to magnetic ISM dust analogue |
en_US |
dc.type |
Journal Paper |
en_US |
dc.relation.journal |
Monthly Notices of the Royal Astronomical Society |
|