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From Wikipedia, the free encyclopedia

NGC 7541
A Hubble Space Telescope (HST) image of NGC 7541
Observation data (J2000 epoch)
ConstellationPisces
Right ascension23h 14m 43.90s[1]
Declination+4° 32′ 03.0″[1]
Redshift0.008936±0.000017[1]
Distance104 Mly (32.0 Mpc)[1]
Characteristics
TypeSB(rs)bc[1]
Size106,000 ly
Apparent size (V)3.2 x 1.0[1]
Notable featuresLots of star-forming regions in spiral arms
Other designations
PGC 70795,[1] UGC 12447,[1] MCG +01-59-017[1]

NGC 7541 is a barred spiral galaxy located around 104 million light-years away in the constellation Pisces.[1] It was discovered in 1785 by William Herschel, and it is 106,000 light-years across.[2] NGC 7541 is known to have lots of star-forming regions.[1]

Characteristics

NGC 7541, like other barred spiral galaxies, has a bar in the center of it.[2] The bar cuts through the center of the galaxy, and into the other side.[3] This type of galaxy is known as "grand design".[1] NGC 7541 is actually observed to have a higher-than-usual star formation rate, adding weight to the theory that spiral bars act as stellar nurseries, corralling and funneling inwards the material and fuel needed to create and nurture new baby stars.[3] NGC 7541 also has an active galactic nuclei, as shown in the HST image.[3][4]

NGC 7541 forms a pair with NGC 7537, a spiral galaxy 127 million light-years away, next to NGC 7541. [4][5] The two galaxies have shown some signs of interaction, as two tidal tails form out of NGC 7541.[3]

One supernova has been observed in NGC 7541. USNOA2 0900-20354891, a type II supernova.[4]

External links

References

  1. ^ a b c d e f g h i j k l "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2023-11-30.
  2. ^ a b "NGC 7541 - Galaxy in Pisces | TheSkyLive.com". theskylive.com. Retrieved 2023-11-30.
  3. ^ a b c d "Bars and Baby Stars". www.spacetelescope.org. Retrieved 2023-11-30.
  4. ^ a b c "NGC 7541 - Galaxy - SKY-MAP". www.wikisky.org. Retrieved 2023-11-30.
  5. ^ "NGC 7537 - Galaxy - SKY-MAP". www.wikisky.org. Retrieved 2023-11-30.
This page was last edited on 4 April 2024, at 13:36
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