3C 351

B1704+608

**Basic Data**
S₁₇₈	Alpha	FR	Class	ID	Spectrum	Best z	mag.	LAS	lg P₁₇₈	D
14.9	0.73	II	CD	QSO		0.371	V = 15.28	75.00	26.52	309.5

Image:

Size:	76.8 × 76.8 arcsec²
LUT:	Logarithmic
Beam:	1.85 arcsec
Frequency:	1417 MHz
Method:	`CLEAN`
Telescope:	VLA A+B
Credits:	Leahy & Perley (1991), R. A. Laing (priv comm)

The mottling in the fainter regions is an artifact of the imaging process, caused by the very bright northern hotspots.

See also the high-resolution image on Alan Bridle's 3C 351 Page.

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Page created: 1998 Mar 12 22:27:14