Loading…

Hydrogenated Polycyclic Aromatic Hydrocarbons and the 2940 and 2850 Wavenumber (3.40 and 3.51 micron) Infrared Emission Features

The 3150-2700 cm-1 (3.17-3.70 microns) range of the spectra of a number of Ar-matrix-isolated PAHs containing excess H atoms (Hn-PAHs) are presented. This region covers features produced by aromatic and aliphatic C-H stretching vibrations as well as overtone and combination bands involving lower lyi...

Full description

Saved in:
Bibliographic Details
Published in:The Astrophysical journal 1996-12, Vol.472 (2), p.L127-L130
Main Authors: Bernstein, Max P, Sandford, Scott A, Allamandola, Louis J
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c435t-9241f7d55af08f7820248598947d573b3ec5cb5e716d0a8b407c6eb5df0cef073
cites cdi_FETCH-LOGICAL-c435t-9241f7d55af08f7820248598947d573b3ec5cb5e716d0a8b407c6eb5df0cef073
container_end_page L130
container_issue 2
container_start_page L127
container_title The Astrophysical journal
container_volume 472
creator Bernstein, Max P
Sandford, Scott A
Allamandola, Louis J
description The 3150-2700 cm-1 (3.17-3.70 microns) range of the spectra of a number of Ar-matrix-isolated PAHs containing excess H atoms (Hn-PAHs) are presented. This region covers features produced by aromatic and aliphatic C-H stretching vibrations as well as overtone and combination bands involving lower lying fundamentals. The aliphatic C-H stretches in molecules of this type having low to modest excess H coverage provide excellent fits to a number of the weak emission features superposed on the plateau between 3080 and 2700 cm-1 (3.25 and 3.7 microns) in the spectra of many planetary nebulae, reflection nebulae, and H II regions. Higher H coverage is implied for a few objects. We compare these results in context with the other suggested identifications of the emission features in the 2950-2700 cm-1 (3.39-3.70 microns) region and briefly discuss their astrophysical implications.
doi_str_mv 10.1086/310376
format article
fullrecord <record><control><sourceid>proquest_iop_p</sourceid><recordid>TN_cdi_iop_primary_10_1086_310376</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>78770122</sourcerecordid><originalsourceid>FETCH-LOGICAL-c435t-9241f7d55af08f7820248598947d573b3ec5cb5e716d0a8b407c6eb5df0cef073</originalsourceid><addsrcrecordid>eNp1kUtLxDAUhYMovv0JEjeiyIx5TtLlIL5gQBeKy5CmN1ppmzFphdn5043OgC50lZubj3NPzkXogJIxJXpyzinharKGtqnkeiS4VOu_6i20k9IrIUSwothEW5RKQZmQ2-jjZlHF8Ayd7aHC96FZuIVraoenMbS2z8U34GwsQ5ew7SrcvwBmhSDfF6YlwU_2HbqhLSHiEz5evfCxpLitXQzdKb7tfLQxT7hs65Tq0OErsP0QIe2hDW-bBPurcxc9Xl0-XNyMZnfXtxfT2cjlD_SjggnqVSWl9UR7pRlhQstCFyI3FS85OOlKCYpOKmJ1KYhyEyhl5YkDTxTfRcdL3XkMbwOk3mQnDprGdhCGZJRWilDGfsDsPKUI3sxj3dq4MJSYr6zNMusMHq4Uh7KF6gdbhZuBoyVQh_n_Imd_MHlv5mtvRihmmJlRpsy88vwTfGWN0w</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>78770122</pqid></control><display><type>article</type><title>Hydrogenated Polycyclic Aromatic Hydrocarbons and the 2940 and 2850 Wavenumber (3.40 and 3.51 micron) Infrared Emission Features</title><source>EZB Electronic Journals Library</source><creator>Bernstein, Max P ; Sandford, Scott A ; Allamandola, Louis J</creator><creatorcontrib>Bernstein, Max P ; Sandford, Scott A ; Allamandola, Louis J</creatorcontrib><description>The 3150-2700 cm-1 (3.17-3.70 microns) range of the spectra of a number of Ar-matrix-isolated PAHs containing excess H atoms (Hn-PAHs) are presented. This region covers features produced by aromatic and aliphatic C-H stretching vibrations as well as overtone and combination bands involving lower lying fundamentals. The aliphatic C-H stretches in molecules of this type having low to modest excess H coverage provide excellent fits to a number of the weak emission features superposed on the plateau between 3080 and 2700 cm-1 (3.25 and 3.7 microns) in the spectra of many planetary nebulae, reflection nebulae, and H II regions. Higher H coverage is implied for a few objects. We compare these results in context with the other suggested identifications of the emission features in the 2950-2700 cm-1 (3.39-3.70 microns) region and briefly discuss their astrophysical implications.</description><identifier>ISSN: 1538-4357</identifier><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1086/310376</identifier><identifier>PMID: 11541245</identifier><language>eng</language><publisher>United States: IOP Publishing</publisher><subject>Astronomy - methods ; Extraterrestrial Environment ; Hydrocarbons, Alicyclic - chemistry ; Hydrogen - chemistry ; Polycyclic Aromatic Hydrocarbons - analysis ; Polycyclic Aromatic Hydrocarbons - chemistry ; Space life sciences ; Spectrophotometry, Infrared</subject><ispartof>The Astrophysical journal, 1996-12, Vol.472 (2), p.L127-L130</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c435t-9241f7d55af08f7820248598947d573b3ec5cb5e716d0a8b407c6eb5df0cef073</citedby><cites>FETCH-LOGICAL-c435t-9241f7d55af08f7820248598947d573b3ec5cb5e716d0a8b407c6eb5df0cef073</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/11541245$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Bernstein, Max P</creatorcontrib><creatorcontrib>Sandford, Scott A</creatorcontrib><creatorcontrib>Allamandola, Louis J</creatorcontrib><title>Hydrogenated Polycyclic Aromatic Hydrocarbons and the 2940 and 2850 Wavenumber (3.40 and 3.51 micron) Infrared Emission Features</title><title>The Astrophysical journal</title><addtitle>Astrophys J</addtitle><description>The 3150-2700 cm-1 (3.17-3.70 microns) range of the spectra of a number of Ar-matrix-isolated PAHs containing excess H atoms (Hn-PAHs) are presented. This region covers features produced by aromatic and aliphatic C-H stretching vibrations as well as overtone and combination bands involving lower lying fundamentals. The aliphatic C-H stretches in molecules of this type having low to modest excess H coverage provide excellent fits to a number of the weak emission features superposed on the plateau between 3080 and 2700 cm-1 (3.25 and 3.7 microns) in the spectra of many planetary nebulae, reflection nebulae, and H II regions. Higher H coverage is implied for a few objects. We compare these results in context with the other suggested identifications of the emission features in the 2950-2700 cm-1 (3.39-3.70 microns) region and briefly discuss their astrophysical implications.</description><subject>Astronomy - methods</subject><subject>Extraterrestrial Environment</subject><subject>Hydrocarbons, Alicyclic - chemistry</subject><subject>Hydrogen - chemistry</subject><subject>Polycyclic Aromatic Hydrocarbons - analysis</subject><subject>Polycyclic Aromatic Hydrocarbons - chemistry</subject><subject>Space life sciences</subject><subject>Spectrophotometry, Infrared</subject><issn>1538-4357</issn><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1996</creationdate><recordtype>article</recordtype><recordid>eNp1kUtLxDAUhYMovv0JEjeiyIx5TtLlIL5gQBeKy5CmN1ppmzFphdn5043OgC50lZubj3NPzkXogJIxJXpyzinharKGtqnkeiS4VOu_6i20k9IrIUSwothEW5RKQZmQ2-jjZlHF8Ayd7aHC96FZuIVraoenMbS2z8U34GwsQ5ew7SrcvwBmhSDfF6YlwU_2HbqhLSHiEz5evfCxpLitXQzdKb7tfLQxT7hs65Tq0OErsP0QIe2hDW-bBPurcxc9Xl0-XNyMZnfXtxfT2cjlD_SjggnqVSWl9UR7pRlhQstCFyI3FS85OOlKCYpOKmJ1KYhyEyhl5YkDTxTfRcdL3XkMbwOk3mQnDprGdhCGZJRWilDGfsDsPKUI3sxj3dq4MJSYr6zNMusMHq4Uh7KF6gdbhZuBoyVQh_n_Imd_MHlv5mtvRihmmJlRpsy88vwTfGWN0w</recordid><startdate>19961201</startdate><enddate>19961201</enddate><creator>Bernstein, Max P</creator><creator>Sandford, Scott A</creator><creator>Allamandola, Louis J</creator><general>IOP Publishing</general><scope>CGR</scope><scope>CUY</scope><scope>CVF</scope><scope>ECM</scope><scope>EIF</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope></search><sort><creationdate>19961201</creationdate><title>Hydrogenated Polycyclic Aromatic Hydrocarbons and the 2940 and 2850 Wavenumber (3.40 and 3.51 micron) Infrared Emission Features</title><author>Bernstein, Max P ; Sandford, Scott A ; Allamandola, Louis J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c435t-9241f7d55af08f7820248598947d573b3ec5cb5e716d0a8b407c6eb5df0cef073</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1996</creationdate><topic>Astronomy - methods</topic><topic>Extraterrestrial Environment</topic><topic>Hydrocarbons, Alicyclic - chemistry</topic><topic>Hydrogen - chemistry</topic><topic>Polycyclic Aromatic Hydrocarbons - analysis</topic><topic>Polycyclic Aromatic Hydrocarbons - chemistry</topic><topic>Space life sciences</topic><topic>Spectrophotometry, Infrared</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bernstein, Max P</creatorcontrib><creatorcontrib>Sandford, Scott A</creatorcontrib><creatorcontrib>Allamandola, Louis J</creatorcontrib><collection>Medline</collection><collection>MEDLINE</collection><collection>MEDLINE (Ovid)</collection><collection>MEDLINE</collection><collection>MEDLINE</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bernstein, Max P</au><au>Sandford, Scott A</au><au>Allamandola, Louis J</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Hydrogenated Polycyclic Aromatic Hydrocarbons and the 2940 and 2850 Wavenumber (3.40 and 3.51 micron) Infrared Emission Features</atitle><jtitle>The Astrophysical journal</jtitle><addtitle>Astrophys J</addtitle><date>1996-12-01</date><risdate>1996</risdate><volume>472</volume><issue>2</issue><spage>L127</spage><epage>L130</epage><pages>L127-L130</pages><issn>1538-4357</issn><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>The 3150-2700 cm-1 (3.17-3.70 microns) range of the spectra of a number of Ar-matrix-isolated PAHs containing excess H atoms (Hn-PAHs) are presented. This region covers features produced by aromatic and aliphatic C-H stretching vibrations as well as overtone and combination bands involving lower lying fundamentals. The aliphatic C-H stretches in molecules of this type having low to modest excess H coverage provide excellent fits to a number of the weak emission features superposed on the plateau between 3080 and 2700 cm-1 (3.25 and 3.7 microns) in the spectra of many planetary nebulae, reflection nebulae, and H II regions. Higher H coverage is implied for a few objects. We compare these results in context with the other suggested identifications of the emission features in the 2950-2700 cm-1 (3.39-3.70 microns) region and briefly discuss their astrophysical implications.</abstract><cop>United States</cop><pub>IOP Publishing</pub><pmid>11541245</pmid><doi>10.1086/310376</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1538-4357
ispartof The Astrophysical journal, 1996-12, Vol.472 (2), p.L127-L130
issn 1538-4357
0004-637X
1538-4357
language eng
recordid cdi_iop_primary_10_1086_310376
source EZB Electronic Journals Library
subjects Astronomy - methods
Extraterrestrial Environment
Hydrocarbons, Alicyclic - chemistry
Hydrogen - chemistry
Polycyclic Aromatic Hydrocarbons - analysis
Polycyclic Aromatic Hydrocarbons - chemistry
Space life sciences
Spectrophotometry, Infrared
title Hydrogenated Polycyclic Aromatic Hydrocarbons and the 2940 and 2850 Wavenumber (3.40 and 3.51 micron) Infrared Emission Features
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T07%3A29%3A11IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_iop_p&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Hydrogenated%20Polycyclic%20Aromatic%20Hydrocarbons%20and%20the%202940%20and%202850%20Wavenumber%20(3.40%20and%203.51%20micron)%20Infrared%20Emission%20Features&rft.jtitle=The%20Astrophysical%20journal&rft.au=Bernstein,%20Max%20P&rft.date=1996-12-01&rft.volume=472&rft.issue=2&rft.spage=L127&rft.epage=L130&rft.pages=L127-L130&rft.issn=1538-4357&rft.eissn=1538-4357&rft_id=info:doi/10.1086/310376&rft_dat=%3Cproquest_iop_p%3E78770122%3C/proquest_iop_p%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c435t-9241f7d55af08f7820248598947d573b3ec5cb5e716d0a8b407c6eb5df0cef073%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=78770122&rft_id=info:pmid/11541245&rfr_iscdi=true