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First evidence of the possible detection of diffuse circumstellar bands in AGB descendants

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dc.contributor.author Di­az-Luis, J. J
dc.contributor.author Garcia-Hernandez, D. A
dc.contributor.author Kameswara Rao, N
dc.contributor.author Manchado, A
dc.contributor.author Cataldo, F
dc.date.accessioned 2020-11-17T02:26:12Z
dc.date.available 2020-11-17T02:26:12Z
dc.date.issued 2016-06
dc.identifier.citation Memorie della Societa Astronomica Italiana, Vol. 87, No. 2, pp. 295-298 en_US
dc.identifier.issn 1824-016X
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7020
dc.description Restricted Access © Societa Astronomica Italiana http://sait.oat.ts.astro.it/MmSAI/87/PDF/295.pdf en_US
dc.description.abstract The short transition phase between asymptotic giant branch stars (AGB; when circumstellar envelopes rich in small organic molecules are efficiently created) and planetary nebulae (PNe) represents a most active phase of molecular synthesis. Different complex organic molecules - e.g., polycyclic aromatic hydrocarbons and fullerenes - have been proposed as carriers of the enigmatic diffuse interstellar bands (DIBs). If the DIBs arise from such large carbon-based molecules, then they are also expected to be present in the circumstellar shells around C-rich AGB descendants; i.e., post-AGB stars and young PNe. Diffuse circumstellar bands (DCBs) in absorption have been unsuccessfully search for more than 40 years; the main difficulty being to distinguish the DCBs from the DIBs. Here we present a detailed DIB radial velocity analysis and a complete search of diffuse bands towards three young PNe (Tc 1, M 1-20, and IC 418) containing fullerenes. Interestingly, we report the first possible detection of two DCBs at 4428 and 5780 Å in the fullerene-rich circumstellar environment around PN Tc 1. This possible detection of DCBs in an environment rich in fullerenes and fullerene-related molecules could provide a link between fullerene compounds and some of the DIB carriers. en_US
dc.language.iso en en_US
dc.publisher Societa Astronomica Italiana en_US
dc.subject Astrochemistry en_US
dc.subject Line: identification en_US
dc.subject Circumstellar matter en_US
dc.subject ISM: molecules en_US
dc.subject Planetary Nebulae: individual: Tc 1, M 1-20, IC 418 en_US
dc.title First evidence of the possible detection of diffuse circumstellar bands in AGB descendants en_US
dc.type Article en_US


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