57 citations · 188 across the 9 of their papers we have counts for
9 papers
Unusual Infrared Emission toward Sgr B2: Possible Planar C
X. H. Chen, F. Y. Xiang, X. J. Yang +1
Interstellar graphene could be present in the interstellar medium (ISM), resulting from the photochemical processing of polycyclic aromatic hydrocarbon (PAH) molecules and/or colli…
The Carriers of the "Unidentified" Infrared Emission Features: Clues from Polycyclic Aromatic Hydrocarbons with Aliphatic Sidegroups
Xuejuan Yang, R. Glaser, Aigen Li +1
The "unidentified" infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 m are ubiquitously seen in various astrophysical regions. The UIE features are characteristic…
On the Aliphatic versus Aromatic Content of the Carriers of the "Unidentified" Infrared Emission Features
Xuejuan Yang, Rainer Glaser, Aigen Li +1
Although it is generally accepted that the so-called "unidentified" infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 micrometer are characteristic of the stretching…
The C--H Stretching Features at 3.2--3.5 Micrometer of Polycyclic Aromatic Hydrocarbons with Aliphatic Sidegroups
Xuejuan Yang, Aigen Li, Rainer Glaser +1
The so-called unidentified infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 micrometer are ubiquitously seen in a wide variety of astrophysical regions. The UIE fea…
High Spatial Resolution Spectroscopy of G292.0+1.8 with Chandra
Xue-Juan Yang, Xiaoqin Liu, Shun-yu Li +1
We present high spatial resolution X-ray spectroscopy of supernova remnant G292.0+1.8 with the {\sl Chandra} observations. The X-ray emitting region of this remnant was divided int…
The Carriers of the Interstellar Unidentified Infrared Emission Features: Constraints from the Interstellar C-H Stretching Features at 3.2-3.5 Micrometers
X. J. Yang, R. Glaser, Aigen Li +1
The unidentified infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 micrometer, commonly attributed to polycyclic aromatic hydrocarbon (PAH) molecules, have been rece…