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NGC 110


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Radio absorption by the intergalactic medium
The IR-radio correlation for spiral galaxies has been used to measurethe absorption of 1.49-GHz radiation by the intergalactic medium.Contrary to conventional expectation, a sample of 237 galaxies shows astrong inverse correlation of radio luminosity (at a given IRluminosity) with distance, Lr = about D exp -0.4, over a range ofdistances from 0.7-55 Mpc. Strong absorption by the intergalactic mediumis the only reasonable explanation of this correlation, which isstatistically significant at the 2 x 10 to the -12th level.

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Observation and Astrometry data

Constellation:Cassiopeia
Right ascension:00h27m18.00s
Declination:+71°24'00.0"
Apparent magnitude:99.9

Catalogs and designations:
Proper Names   (Edit)
NGC 2000.0NGC 110

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