A SDSS survey image and from the Hubble Space Telescope, showed that NGC 7609 is interacting with nearby galaxy, PGC 71077 (HCG 95C) whose spiral arms is currently being absorbed by the larger entity.[7] A double-nuclei is present in HCG 95C, which is considered a merger remanent of two disk galaxies.[7] Two tidal tails[8] are also found in NGC 7609 and HCG 95C region, which seems to connect together,[9] and there is a linear bridge between two galaxies indicating nuclear activity is taking place in HCG 95C.[10] From the study written from Vilchez & Iglesias-Paramo in 1998, Hα emission is detected in the nuclei of both galaxies and also the larger tidal tails (the eastern tail).[11]
From the spatial profiles, this indicates non-nuclear starburst activity triggered by tidal forces while nuclear spectrum indicates non thermal activity. From the further IUE observations of HCG 95C, it presents a featureless continuum with transient outburst captured in one observation, showing galactic emission of red-shifted N v (1240 A) and C IV (1550 A). This result depicts HCG 95C is in the early stages of merging with NGC 7609.[10]
According to another study, it is suggested that a dwarf galaxy might have been created at the tip of the northern tidal tails.[12]
Hickson 95 group
NGC 7609 is a member of Hickson Compact Group 95.[13][14] There are total of four galaxies in the group, in which the members are PGC 71074, PGC 71077 and PGC 71080.[15][16] Of all the four galaxies, PGC 71080 (HCG 95B) is a foreground galaxy, as its line-of-sight velocity of 8000 km/s significantly differs from the velocity of the other members per published by Hickson et al.[17]
Presence of ultra-diffuse galaxies around HCG 95
A study mentions there is a detection of 89 candidate ultra-diffuse galaxies (UDGs), around NGC 7609 and HCG 95, in which one is linked with. It is a gas-rich galaxy with H i mass 1.1 x 10 M⊙, detected by Very Large Array, and has a stellar mass of M 1.8 x 10 M⊙.[18] This indicates that UDGs partially overlap with population of nearly dark galaxies found in deep H I surveys. The results show high abundance of blue UDGs in the HCG 95 field is favored by the poor galaxy cluster environment residing in H I-rich large-scale structures.[18]
Supernova
One supernova has been observed in NGC 7609. SN 1973M (type unknown, mag. 19) was discovered by Charles Kowal on 8 June 1973.[19][20]
^de Oliveira, C. Mendes; Da Rocha, C.; Rabaça, C. R.; Pereira, D. N. E.; Bolte, M. (2003), "Optical Diffuse Light in Nearby Compact Groups", Extragalactic Globular Cluster Systems, Eso Astrophysics Symposia, pp. 191–195, arXiv:astro-ph/0210576, doi:10.1007/10857603_31, ISBN3-540-40472-4
