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Radio galaxy and merger remnant From Wikipedia, the free encyclopedia
Arp 187 is a radio galaxy and merger remnant located in the constellation Eridanus. It is an interacting galaxy pair (MCG-02-13-040).[2] It is included in the Atlas of Peculiar Galaxies in the category galaxies with narrow filaments.
Arp 187 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Eridanus |
Right ascension | 5h 03m 53s [1] |
Declination | −10° 14′ 51″ [1] |
Redshift | 12095 ± 45 km/s [1] |
Apparent magnitude (V) | 15.3 [1] |
Characteristics | |
Type | Radio Galaxy [1] |
Apparent size (V) | 0.8 x 0.6 [1] |
Other designations | |
PGC 16691 [1] |
The galaxy has two prominent radio lobes, however the emission of its AGN in X-ray is low, and so is the thermal output of the AGN torus as observed in infrared, suggesting that it has been quenched. The detection of a narrow line region (with dimensions up to 10 kpc) with still active emission mean that the AGN was still active up to at least 104-5 years ago. In the nucleus of Arp 187 is predicted to lie a supermassive black hole (SMBH) with estimated mass around 6.7 × 108 M☉.[3] Further observations of such a SMBH with a quenched AGN were published in 2019.[4][5][6]
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