NGC 7496
Apparent magnitude (V) | 11.1 |
---|---|
Characteristics | |
Type | (R':)SB(rs)bc [1] |
Apparent size (V) | 3.3′ × 3.0′[1] |
Notable features | Seyfert galaxy, starburst galaxy |
Other designations | |
ESO 291- G001, VV 771, MCG -07-47-020, PGC 70588[1] |
NGC 7496 is a barred spiral galaxy located in the constellation Grus. It is located at a distance of about 60 million light-years from Earth, which, given its apparent dimensions, means that it is 75,000 light years across. It was discovered by John Herschel on September 5, 1834.[3] It is a type 2 Seyfert galaxy with high star formation rate around the nucleus.[4]
Characteristics
The nucleus of the galaxy has been found to be
NGC 7496 was one of the first galaxies to be examined by the
Clumpy ultraviolet emission has been observed from the spiral arms of the galaxy. Massive stellar complexes are present in the north arm and regions with young stellar complexes are present in the end of both arms. The age of the stars in these complexes is estimated to be less than 200 million years. Photometry in various wavelengths indicates that there is very cold dust in the galaxy.[7]
Nearby galaxies
NGC 7496 is a member of the NGC 7582 galaxy group.
Gallery
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The galaxy inmid infrared by the James Webb Space Telescope[11]
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The galaxy in near infrared by JWST
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The galaxy in ultraviolet by GALEX
See also
- NGC 7479 - a similar barred galaxy
References
- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 7496. Retrieved 2019-01-18.
- ^ .
- ^ Seligman, Courtney. "NGC 7496 (= PGC 68165)". Celestial Atlas. Retrieved 19 November 2018.
- doi:10.1086/501529.
- doi:10.1086/191771.
- .
- .
- ^ S2CID 119194025. Archived from the originalon 31 January 2016. Retrieved 20 January 2019.
- ISBN 978-1-4419-1777-5.
- Bibcode:1993A&AS..100..493F.)
{{cite journal}}
: CS1 maint: multiple names: authors list (link - ^ "NGC 7496 (MIRI Image)". www.esawebb.org. 16 February 2023. Retrieved 18 November 2023.
External links
- NGC 7496 on
- NGC 7496 on SIMBAD