In the Vinony graph
Vinony's link graph records 549 inbound references to Q1106223, and connects out to Q1105445, epoch and NGC 3977.
Vinony files it under Irregular galaxies, M94 Group and NGC objects.
Vinony links it to 31 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- AG?
- Redshift
- z = 0.0007838756237156573
- Morphology
- dIA
- Coordinates
- RA 174.0240° · Dec 45.2842°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Ursa Major
- Right ascension
- 11 36 05
- Declination
- +45 ° 17 ′ 02 ″
- Heliocentric radial velocity
- 229 ± 4 km/s
- Distance
- 10 Mly (3.2 Mpc )
- Type
- ImIII/BCD
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 3.0
- Image
- NGC 3741.png
Show 9 more facts
- galaxy morphological type
- Im
- catalog code
- SPB 158
- Commons category
- NGC 3741
- time of discovery or invention
- 1828-00-00
- apparent magnitude
- 15.16
- right ascension
- 174.0239740
- declination
- 45.2841550
- redshift
- 0.000764
- radial velocity
- 230
via Wikidata · CC0
~1 min read
Encyclopedic overview
NGC 3741 is an irregular galaxy in the constellation Ursa Major. It was discovered by John Herschel on March 19, 1828. At a distance of about 10 million light-years (3.2 Mpc), it is located in the M94 Group. It is relatively undisturbed by other galaxies.
NGC 3741 is an unusual galaxy in several aspects. It has a disk of neutral hydrogen (H I) that is extremely wide, extending some 23,000 light-years (7 kpc). The disk is strongly but symmetrically warped. With a mass-to-light ratio of MT/LB ~ 149, it is highly rich in dark matter.
Excerpted from Wikipedia’s “Q1106223” article, available under the CC BY-SA 4.0 licence.
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