Sagittarius A & Halo |
 | Minimum credit line: Image courtesy of NRAO/AUI
(for details, see .
|
This is a pseudo-color representation of Sgr A and its halo at 90 cm (332 MHz). The coding of the brightness scale is indicated by the color bar. Sgr A East is a non-thermal shell source that could be a supernova remnant or a very low-luminosity example of a radio component associated with the active nucleus of a spiral galaxy. The most dramatic aspect of the new 332 MHz observations is the appearance of the Sgr A West spiral features in absorption against Sgr A East. Based on these results, Sgr A East is situated behind Sgr A West, the center of the galaxy. The halo is in front of or surrounds the former sources. The HII regions to the east of Sgr A East are probably associated with the 50 km/s molecular cloud. The 7 arcmin halo (20 pc) has a non-thermal spectrum with turn-over below 1 GHz. Investigator(s): W. M. Goss, K. R. Anantharamaiah, R. D. Ekers, and A. Pedlar This image is available in the following downloadable versions:
- 480 x 520
- 900 x 975
- 1939 x 2100
If you would like to obtain a higher resolution version of this image,
please contact .
- Read the
- Up one level for more info on
- For unfamiliar terms, visit the NRAO
|
Telescope
|
VLA
|
|
Date of Observation
|
1987-00-00
|
|
Type of Observation
|
Continuum Observations
|
|
Band
|
P
|
|
Wavelength
|
90 cm
|
|
Frequency
|
330 MHz
|
|
Center of Image
|
RA: 17:43:15.00, Dec: -28:52:0.00 (J2000)
|
|
Field of View
|
0.2167 x 0.2167 degrees
|
|
Technical Caption
|
VLA in A,B,C,D configuration using 15 antennas. Angular resolution is 12" x 12".
|
- Astronomical database entries for Sgr A
- Query for more Sgr A data
SEARCH THE IMAGE GALLERY
To search the Image Gallery for other images of Sgr A, click the Submit button.
To search the Image Gallery for similar images, click the Submit button.
For more search options, please use our form.
|
|
|