期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 441, 期 4, 页码 2996-3008出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stu774
关键词
techniques: imaging spectroscopy; proper motions; ISM: individual objects: Cassiopeia A; ISM: supernova remnants
资金
- Canada Research Chair programme
- Natural Sciences and Engineering Research Council of Canada
- Fonds de Recherche du Quebec-Nature et Technologies (FRQ-NT)
- Ministere de l'Enseignement superieur, de la Recherche, de la Science et de la Technologie (Quebec - PCUC program)
We used the imaging Fourier transform spectrometer SpectromStre Imageur de l'Observatoire du Mont-M,gantic (SpIOMM) to obtain hyperspectral cubes of the young supernova remnant Cassiopeia A (Cas A). The cubes contain over 5000 spatially resolved spectra covering the spectral range 6480-7050 . We first investigate the slow-moving N-rich quasi-stationary flocculi by measuring their radial velocity as well as the [N ii] lambda 6583/H alpha ratio. No correlation between their radial velocity and [N ii] lambda 6583/H alpha ratio with their location has been found. We used multi-epoch observations from the Hubble Space Telescope to create a proper motion map, showing the displacement of several filaments over the most part of Cas A. Combining data from SpIOMM and Hubble, we re-evaluate the distance to Cas A and obtained 3.33 +/- A 0.10 kpc, which is in good agreement with previous estimates. Finally, we obtain a three-dimensional spatial view of the [S ii] lambda lambda 6716, 6731 emissions showing their location, expansion velocity and the [S ii] doublet line ratio for multiple locations in the remnant. The velocity asymmetry reported by previous analyses is clearly visible. Also, the [S ii] doublet ratio (with a mean value of 0.5 +/- A 0.2) indicates a very high and variable electronic density throughout the remnant.
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