X-Ray Nova GRO J1655-40 |
 | Minimum credit line: Image courtesy of NRAO/AUI
(for details, see .
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A time ordered sequence of images of the microquasar
GRO J1655-10, with earlier times at the top and later times
underneath.
This sequence covers a month in the life of the microquasar,
as imaged by the VLBA. GRO J1655-40 is a binary
system in which the outer envelope of the normal star is overflowing
onto its black hole companion. The accreting matter swirls into
a rapidly rotating disk as it falls towards the black hole; near the
center, some of this matter is "squirted out" perpendicular to the disk,
at relativistic speeds (i.e, speeds approaching the speed of light).
The radio emission associated with these relativistic jets is what
we see here. The intrinsic speed of these jets is about 90% of the
speed of light. Because the jets are moving almost as fast as the
radiation they emit, the approaching jet appears to move even faster,
and the apparent motions range up to 1.3 times the speed of light.
See
http://www.astro.soton.ac.uk/~rih/j1655.html for an
artist's impression of this system. Investigator(s): Robert Hjellming and Michael Rupen This image is available in the following downloadable versions: If you would like to obtain a higher resolution version of this image,
please contact .
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Telescope
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VLBA
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Date of Observation
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1994-09-00
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Type of Observation
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Continuum Observations
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Band
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L
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Wavelength
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20 cm
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Frequency
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1.4 GHz
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Center of Image
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RA: 16:54:0.14, Dec: -39:50:44.90 (J2000)
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Field of View
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0.0008 x 0.0001 degrees
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Technical Caption
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VLBA images at 1.6 GHz. Images made from data collected
in August and September, 1994. Top image from Aug 18-19;
next one from Aug 22-23; next Aug 25-26; next Aug 25-26;
next Sep 1-2; next Sep 8-9; next Sep 12-13; and last
Sep 20-21.
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- Astronomical database entries for GRO J1655-40
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