2022MNRAS.517.4845R


Query : 2022MNRAS.517.4845R

2022MNRAS.517.4845R - Mon. Not. R. Astron. Soc., 517, 4845-4855 (2022/December-3)

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

ROY A., SINGH S.V., MEKA J.K., RAMACHANDRAN R., SAHU D., GAUTAM A., VIJAY T., VISHAKANTAIAH J., JANARDHAN P., RAJASEKHAR B.N., BHARDWAJ A., MASON N.J. and SIVARAMAN B.

Abstract (from CDS):

The fate of organometallic dust subjected to extreme conditions, especially the shock fronts, in the interstellar medium (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 the organometallic compound ferrocene under terrestrial conditions. In our experiment we subjected ferrocene, a possible proxy of such dust, to ∼5.6 Mach (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.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): Astrochemistry - shock waves - methods: laboratory - dust, extinction

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0

Query : 2022MNRAS.517.4845R

Basic data :
TMC-1 -- Molecular Cloud
Other object types:
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PoC (MLB,[MOH94]), MoC (TMC), Cld (HCL)
ICRS coord. (ep=J2000) :
04 41 45.9 +25 41 27 [ ] D 1983ApJ...264..517M
FK4 coord. (ep=B1950 eq=1950) :
04 38 42.0 +25 35 45 [ ]
Gal coord. (ep=J2000) :
174.3852 -13.4312 [ ]
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Hierarchy : number of linked objects
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HCL 2 MLB 3-28 TMC-1 [MOH94] 6

References (1872 between 1850 and 2026) (Total 1872)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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