Markarian 348 (NGC 262) - Optical/Radio Composite
Description
Composite optical-HI image of Markarian 348, a Type 2 Seyfert Galaxy. The cold, neutral hydrogen is shown in blue; the stars in the galaxy and the surrounding field are shown in red. The gas distribution spans a diameter of roughly 290 kpc, assuming a distance of 95 Mpc for Mkn 348, and is one of the largest such structures known. The fuzzy, red blob to the right of the main optical galaxy but embedded in the central, blue HI gas has the same redshift as Mkn 348 and is thought to be tidally disrupting the main galaxy. This tidal disruption may be responsible for the excess energy in the galaxy's Seyfert nucleus.
Optical data was obtained from four deep Palomar Schmidt images (90-minute exposures) taken with broadband filters centered at approximately 4800 A and 6500 A. The HI 21-cm emission line radio data was taken at the VLA using 25 antennas for 6 hours in the C-configuration and for 4 hours in the D-configuration. Sum of 13 velocity channels (4604 to 4476 km/s)
Creator
Legacy Astronomical Images
Rights
NRAO/AUI/NSF does not hold full copyright for this image. Contact the archivist for details.
Type
Legacy Astronomical Image
Object Name
NGC262
Investigators
S.M. Simkin, J.H. van Gorkom, H.J. Su
Telescope
Very Large Array (VLA)
Observation Date
1984-08-16
Type of Observation
spectral line
Wavelength
21 cm
Frequency
1420.4 MHz
Species
HI
Center of Image
RA 0:48:47.144, Dec: 31:57:25.096
Field of View
0.500000 x 0.500000 degrees
Link to journal article
Notes
Contact the archivist for a high resolution tif of this image.
Series
Active Galactic Nuclei Series
Unit
Seyferts Unit
Citation
Legacy Astronomical Images, “Markarian 348 (NGC 262) - Optical/Radio Composite,” NRAO/AUI Archives, accessed December 24, 2024, https://www.nrao.edu/archives/items/show/33412.