Astronomy:NGC 3200
| NGC 3200 | |
|---|---|
 NGC 3200 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Hydra |
| Right ascension | 10h 18m 36.5578s |
| Declination | −17° 58′ 56.973″ |
| Apparent magnitude (B) | 12.92 |
| Characteristics | |
| Type | SAc |
| Other designations | |
| ESO 567- G 045, MCG-03-26-037, PGC 30108 | |
NGC 3200 is a large spiral galaxy located in the constellation Hydra. Its velocity relative to the cosmic microwave background is 3,877 ± 25 km/s, which corresponds to a Hubble distance of 57.2 ± 4.0 Mpc (~187 million ly). NGC 3200 was discovered by American astronomer Edward Singleton Holden in 1882.[1]
The luminosity class of NGC 3200 is III and it exhibits a broad HI line.[2]
To date, 21 non-redshift measurements give a distance of 43.086 ± 12.631 Mpc (~141 million ly) which is within the Hubble distance values.[3] Note, however, that the NASA/IPAC database calculates the diameter of a galaxy using the average value of independent measurements, when they exist, and that consequently the diameter of NGC 3200 could be about 116.4 kpc (~380,000 ly ) if the Hubble distance were used to calculate it.[4]
Supernovae
One supernova has been observed in NGC 3200: SN 1953D (type unknown, mag. 19.5) was discovered by Chai on 8 March 1953.[5][6]
See also
External links
References
- ↑ "By Name | NASA/IPAC Extragalactic Database". http://ned.ipac.caltech.edu/byname?objname=NGC+3200&hconst=67.8&omegam=0.308&omegav=0.692&wmap=4&corr_z=1.
- ↑ "NED Query Results for NGC 3200". https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+3200.
- ↑ "Distance Results for NGC 3200". NASA. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+3200.
- ↑ "HyperLeda -object description". http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=ngc%203200.
- ↑ "Other Supernovae images". https://www.rochesterastronomy.org/snimages/snother.html#1953D.
- ↑ "SN 1953D". IAU. https://www.wis-tns.org/object/1953D.
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