Zobrazeno 1 - 10
of 39
pro vyhledávání: '"NEED ULTRAVIOLET EXCITATION"'
Autor:
Li, Aigen, Draine, B. T.
One of the major challenges to identification of the 3.3, 6.2, 7.7, 8.6, and 11.3um interstellar IR emission bands with polycyclic aromatic hydrocarbon (PAH) molecules has been the recent detection of these bands in regions with little UV illuminatio
Externí odkaz:
http://arxiv.org/abs/astro-ph/0201060
We present the results of imaging spectroscopy of the reflection nebula vdB 133, obtained with the infrared camera and circular variable filter wheel on the Infrared Space Observatory (ISO). Our observations reveal the infrared emission features (IEF
Externí odkaz:
http://arxiv.org/abs/astro-ph/9711200
Akademický článek
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Akademický článek
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Autor:
Aigen Li, Bruce T. Draine
Publikováno v:
The Astrophysical Journal. 572:232-237
One of the major challenges to identification of the 3.3, 6.2, 7.7, 8.6, and 11.3um interstellar IR emission bands with polycyclic aromatic hydrocarbon (PAH) molecules has been the recent detection of these bands in regions with little UV illuminatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::98a46230b592069ba850fe821ed01aad
https://doi.org/10.1086/340285
https://doi.org/10.1086/340285
Publikováno v:
The Astrophysical Journal. 493:L109-L112
We present the results of imaging spectroscopy of the reflection nebula vdB 133, obtained with the infrared camera and circular variable filter wheel on the Infrared Space Observatory (ISO). Our observations reveal the infrared emission features (IEF
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d521bad9f880d99c90c2dd4783c78808
https://doi.org/10.1086/311136
https://doi.org/10.1086/311136
Autor:
and, Aigen Li
Publikováno v:
The Astrophysical Journal; June 2002, Vol. 572 Issue: 1 p232-237, 6p
Publikováno v:
The Astrophysical Journal. 673(2):798-809
H I features near young star clusters in M81 are identified as the photodissociated surfaces of giant molecular clouds (GMCs) from which the young stars have recently formed. The H I column densities of these features show a weak trend, from undetect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dris___01423::2966bf0f592aa8e52a9c9337c45416e1
https://research.rug.nl/en/publications/847da12a-0253-4fe4-8ce5-d9fc1ecdf686
https://research.rug.nl/en/publications/847da12a-0253-4fe4-8ce5-d9fc1ecdf686
Publikováno v:
The Astrophysical Journal. 613(2):986-1003
Infrared (IR) emission features at 3.3, 6.2, 7.7, 8.6, and 11.3 mum are generally attributed to IR fluorescence from ( mainly) far-ultraviolet (FUV) pumped large polycyclic aromatic hydrocarbon (PAH) molecules. As such, these features trace the FUV s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dris___01423::781d73c892bcbf79614e3d7b1c59437a
https://research.rug.nl/en/publications/2bafe9be-5e6d-4c18-9c1f-966f2fc553cf
https://research.rug.nl/en/publications/2bafe9be-5e6d-4c18-9c1f-966f2fc553cf
Publikováno v:
Astrophysical Journal, 613(2), 986-1003. IOP PUBLISHING LTD
Infrared (IR) emission features at 3.3, 6.2, 7.7, 8.6, and 11.3 mum are generally attributed to IR fluorescence from ( mainly) far-ultraviolet (FUV) pumped large polycyclic aromatic hydrocarbon (PAH) molecules. As such, these features trace the FUV s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7fabf3aa7efa8cf9d47478e42e7b18f5
https://doi.org/10.1086/423237
https://doi.org/10.1086/423237