Date and Time of the Query: 2019-08-25 T00:40:55 PDT
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Notes for object IC 0310

5 note(s) found in NED.

1. 2002AJ....124..675C
Re:UGC 02624
Head-tail radio source.

2. 1998A&A...331..475F
Re:IC 0310
3.1. IC 310 - 0313+411
IC 310 is located in the Perseus cluster. Previous observations of this radio
galaxy are listed by Mack et al. (1993), who first mapped the large-scale
structure of this source at a high frequency. The 10.6-GHz map presented here
in Fig. 1 has a higher sensitivity, owing to additional scans. For the spectral
comparison, we used the WSRT maps at 327 and 610 MHz by Sijbring (1993),
convolved to the same resolution of 69".
The trend of the spectral index ({alpha}_0.3_^0.6^ and {alpha}_0.6_^10.6^;
I_{nu}_is proportional to {nu}^-{alpha}^) derived along the maximum brightness
ridge is given in Fig. 5. The low-frequency spectral index {alpha}_0.3_^0.6^ is
0.4, almost constant up to 2' from the core, suggesting that the particles
radiating in this region and at low frequencies have not suffered synchrotron
losses. A clear steepening is visible at high frequencies and with increasing
distance from the core.
The tail is strongly polarized, up to a distance of 3' from the core, with the
polarization percentage increasing along the tail (see Fig. 6). The orientation
of the polarization vectors is perpendicular to the tail (see Fig. 1).

3. 1992A&AS...95..129P
Re:IC 0310
IC 310: No significant deviation from close-to-circular isophotes. The
profile is consistent with an r^1/4^ law in the central 40 arcsec. Note
the RC2 classification: LAR0.

4. 1976RC2...C...0000d
Re:IC 0310
In the Perseus Cluster
Description and Photograph:
P.A.S.P., 80, 129, 1968.
Photometry and Isodensitometry:
A.J., 79, 671, 1974.
Radio Observations:
M.N.R.A.S., 138, 1, 1968.
Nature, 237, 269, 1972.
Astr. Ap., 26, 413, 1973.

5. 1973UGC...C...0000N
Re:UGC 02624
Perseus cluster
Tendency to spiral structure
UGC 02626 at 3.7, 59

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