Polycyclic aromatic hydrocarbons in interstellar medium

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/767

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DC Field	Value	Language
dc.contributor.author	Rastogi, S	-
dc.date.accessioned	2006-03-14T10:16:04Z	-
dc.date.available	2006-03-14T10:16:04Z	-
dc.date.issued	2005-06	-
dc.identifier.citation	BASI, Vol. 33, No. 2, pp. 167-174	en
dc.identifier.uri	http://hdl.handle.net/2248/767	-
dc.description.abstract	Polycyclic Aromatic Hydrocarbons (PAHs) are an important com- ponent of the Interstellar Medium (ISM). They are being used as probes for understanding of process and conditions of different astrophysical environments. The understanding of their IR spectra and its variations with PAH size and ionization state is useful in characterizing the ISM. Spectral features of model graphene sheets and also that of smaller PAH molecules are reported. The variation of intensity with charge state of the molecule shows that cations give a better correlation with observations. The relationship between changes in charge distribution with intensity changes upon ionization has been probed	en
dc.format.extent	261360 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	PAH	en
dc.subject	Aromatic Infrared Bands	en
dc.subject	Interstellar Medium	en
dc.title	Polycyclic aromatic hydrocarbons in interstellar medium	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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