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29 March 2024 |
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Article overview
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White dwarfs with jets as non-relativistic analogues of quasars and microquasars? | R. Zamanov
; M.F. Bode
; P. Marziani
; R.J. Davis
; S.P.S. Eyres
; A. Gomboc
; J. Porter
; A. Skopal
; | Date: |
17 Dec 2004 | Subject: | astro-ph | Abstract: | We explore the similarities between accreting white dwarfs (CH Cyg and MWC 560) and the much more energetic jet sources - quasars and microquasars. To-date we have identified several common attributes: (1) they exhibit collimated outflows (jets); (2) the jets are precessing; (3) these two symbiotic stars exhibit quasar-like emission line spectra; (4) there is a disk-jet connection like that observed in microquasars. Additionally they may have a similar energy source (extraction of rotational energy from the accreting object). Study of the low energy analogues could have important implications for our understanding of their higher energy cousins. | Source: | arXiv, astro-ph/0412462 | Services: | Forum | Review | PDF | Favorites |
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