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[vsnet-alert 1675] Image of the CI Cam Radio Jets (Hjellming)
- Date: Wed, 15 Apr 1998 09:33:00 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 1675] Image of the CI Cam Radio Jets (Hjellming)
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
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Date: Wed, 15 Apr 1998 05:18:37 +0900 (JST)
To: rhjellmi@nrao.edu
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Date: Tue, 14 Apr 1998 13:46:58 -0600
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From: "Robert M. Hjellming (Bob)" <rhjellmi@aoc.nrao.edu>
Cc: rhjellmi@arana.aoc.nrao.edu, amiodusz@arana.aoc.nrao.edu,
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Subject: [vsnet-alert 0] Image of the CI Cam (=XTE J0421+560) Radio Jets April 3, 1998
Errors-To: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
To all of you that I have sent advanced, almost premature, information
during the early days of the CI Cam outburst:
In IAU Circular 6872 we reported that CI Cam was showing S-shaped
"corkscrews" of emission. If you look at the Web page at URL
http://vsnet.aoc.nrao.edu/~rhjellmi/cicam.html
you can see a color version of the April 3.83 UT image made from
VLA 1.3cm data.
We have in hand four additional epochs of VLA images of its
SS433-like rotating corkscrew of emission, and may get another
one this afternoon, if it is not too weak now. The radio
emission is moving out very fast, 54 mas/day on average.
For some components, like the initial ejecta seen in the outer
extremes of the April 3 image, I think the motion was more like
85 mas/day. Thus the 0.15c for a distance of 1 kpc was too small
by a factor of at least 2-2.5. The corkscrew behavior fits
with v in the range 0.3c to 0.4c (if the distance is 1 kpc).
Amy Mioduszewki has made a VLBA image from April 1st data, and
we see a core source with a jet in the "right" direction. The
April 5 VLBA images should be even more interesting.
Cheers, Bob
Return to Daisaku Nogami
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