Methylpolyynes and Small Hydrocarbons in CRL 618

Details Methylpolyynes and Small Hydrocarbons in CRL 618 Methylpolyynes and Small Hydrocarbons in CRL 618

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...546l.127c&link_type=abstract

The Astrophysical Journal, Volume 546, Issue 2, pp. L127-L130.

Astronomy and Astrophysics

Astronomy

52

Stars: Circumstellar Matter, Infrared: General, Ism: Molecules, Line: Profiles, Stars: Individual: Alphanumeric: Crl 618, Stars: Individual: Alphanumeric: Crl 2688, Stars: Individual: Alphanumeric: Ngc 7027

Scientific paper

We report on the detection with the Infrared Space Observatory of strong infrared absorption from NH3 and C2H4 in CRL 618. The observed NH3 and C2H4 bands arise from a region with kinetic temperatures ~=200 K, i.e., the dense gas in the photodissociation region associated to the dense torus surrounding the central star, as was the case for the polyynes and cyanopolyynes (see the companion Letter). Several absorption bands, probably arising from small gas-phase hydrocarbons, are observed between 5.5 and 11 μm. Two of these species have been identified with the 30 m IRAM telescope as the methylpolyynes CH3C2H and CH3C4H. However, the absorption around 6.2 μm is particularly broad and could arise from the combination of these small hydrocarbons and from the aromatic CC stretching of polycyclic aromatic hydrocarbons of moderate size. These bands and those associated to the polyynes, cyanopolyynes, methylpolyynes, and benzene are not present in the infrared spectrum of the asymptotic giant branch star IRC +10216.

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