Uwe Glahn
April 9th, 2018, 09:12 PM
NGC 3165, Holm 173C
RA: 10h 13m 31.4s
Dec: +03° 22’ 30”
Magnitude: 13.9v
NGC 3166, Holm 173A, KPG 228A
RA: 10h 13m 45.5s
Dec: +03° 25’ 23”
Magnitude: 10.5v
NGC 3169, Holm 173B, KPG 228B
RA: 10h 14m 14.7s
Dec: +03° 28’ 01”
Magnitude: 10.3v
In the neighbourhood of the famous galaxies (galaxy-groups) in Leo, the interacting galaxy group Holm 173 aka NGC 3165/3166/3169 is often forgotten. In the northern field of the constellation Sextans the brightest two galaxies are almost a target for the smallest apertures. Larger telescopes shows much detail and so theses galaxies stands not back against their northern colleagues.
The brightest two members NGC 3166 and NGC 3169 were discovered in 1783 from Wilhelm Herschel. NGC 3165 followed in 1856 by William Parsons. In 1937 the Swedish astronomer Erik Holmberg summarized all three mentioned galaxies as a trio [1937AnLun...6....1H]. Karachentsev concentrated on the two brightest members NGC 3166/3169 for the entry in his compilation of galaxy pairs [1972AISAO...7....3K]. Arp, Zwicky, Markarian or Vorontsov-Velyaminov misses to catalogue the group or any individual galaxy.
The similar red shifts (distances ~70 million light-years) and the distorted shapes indicates the gravitational interaction. Also an observed bridge of neutral hydrogen (HI) between the galaxies confirms the common bond between the trio.
The challenges for the galaxies are so different as the used apertures. While small apertures shows the galaxies as small fuzzy patches, mid size telescopes shows the different shapes of all three galaxies as dark lanes in NGC 3169 or the faint bar of NGC 3166. Giant telescopes could perhaps show the extremely faint outer envelope of NGC 3169 or the faint companion galaxy NW of NGC 3166.
DSS blue 20'x20'
2973
sketch: 4" binocular telescope, 55x, NELM 6m5+
2970
sketch: 14.5", 202x, NELM 6m5+, Seeing III
2971
sketch: 27", 172x, NELM 6m5+, Seeing III
2972
Give it a go and let us know!
RA: 10h 13m 31.4s
Dec: +03° 22’ 30”
Magnitude: 13.9v
NGC 3166, Holm 173A, KPG 228A
RA: 10h 13m 45.5s
Dec: +03° 25’ 23”
Magnitude: 10.5v
NGC 3169, Holm 173B, KPG 228B
RA: 10h 14m 14.7s
Dec: +03° 28’ 01”
Magnitude: 10.3v
In the neighbourhood of the famous galaxies (galaxy-groups) in Leo, the interacting galaxy group Holm 173 aka NGC 3165/3166/3169 is often forgotten. In the northern field of the constellation Sextans the brightest two galaxies are almost a target for the smallest apertures. Larger telescopes shows much detail and so theses galaxies stands not back against their northern colleagues.
The brightest two members NGC 3166 and NGC 3169 were discovered in 1783 from Wilhelm Herschel. NGC 3165 followed in 1856 by William Parsons. In 1937 the Swedish astronomer Erik Holmberg summarized all three mentioned galaxies as a trio [1937AnLun...6....1H]. Karachentsev concentrated on the two brightest members NGC 3166/3169 for the entry in his compilation of galaxy pairs [1972AISAO...7....3K]. Arp, Zwicky, Markarian or Vorontsov-Velyaminov misses to catalogue the group or any individual galaxy.
The similar red shifts (distances ~70 million light-years) and the distorted shapes indicates the gravitational interaction. Also an observed bridge of neutral hydrogen (HI) between the galaxies confirms the common bond between the trio.
The challenges for the galaxies are so different as the used apertures. While small apertures shows the galaxies as small fuzzy patches, mid size telescopes shows the different shapes of all three galaxies as dark lanes in NGC 3169 or the faint bar of NGC 3166. Giant telescopes could perhaps show the extremely faint outer envelope of NGC 3169 or the faint companion galaxy NW of NGC 3166.
DSS blue 20'x20'
2973
sketch: 4" binocular telescope, 55x, NELM 6m5+
2970
sketch: 14.5", 202x, NELM 6m5+, Seeing III
2971
sketch: 27", 172x, NELM 6m5+, Seeing III
2972
Give it a go and let us know!