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Radio and X-ray images of the SNR G18.8+0.3 interacting with molecular clouds

Author
TIAN, W. W1 2 ; LEAHY, D. A2 ; WANG, Q. D3
[1] National Astronomical Observatories, CAS, Beijing 100012, China
[2] Department of Physics & Astronomy, University of Calgary, Calgary, Alberta T2N I N4, Canada
[3] Department of Astronomy, University of Massachusetts, 710 North Pleasant Street, Amherst, MA 01003, United States
Source

Astronomy and astrophysics (Berlin. Print). 2007, Vol 474, Num 2, pp 541-547, 7 p ; ref : 1/4 p

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
ISM: structure ISM: supernova remnants galaxies: ISM galaxies: kinematics and dynamics
Keyword (fr)
Basse température Borne inférieure Borne supérieure Cinématique Continuum Densité colonne Dynamique Filament Front densité Galaxies Haute température Imagerie RX Luminosité Nuage moléculaire Plan galactique Reste supernova Spectre émission Température brillance
Keyword (en)
Low temperature Lower bound Upper bound Kinematics Continuum Column density Dynamics Filaments Density front Galaxies High temperature X-ray imaging Luminosity Molecular clouds Galactic planes Supernova remnants Emission spectra Brightness temperature
Keyword (es)
Baja temperatura Cota inferior Cota superior Continuo Densidad columna Frente densidad Alta temperatura Temperatura brillo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19148581

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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