Shock induced transformation of non-magnetic to magnetic ISM dust analogue

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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


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