NGC 3535

In today's article we are going to address the topic of NGC 3535, an issue that has generated interest and debate in different areas. NGC 3535 is a topic that is not limited to a single focus, since it can range from personal, professional, cultural, historical, social or political aspects. It is a topic that has captured the attention of many, and it is important to discuss it from different perspectives to better understand its scope and impact. Throughout this article, we will analyze different aspects related to NGC 3535, exploring its implications and possible solutions.

NGC 3535
The spiral galaxy NGC 3535.
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 08m 33.9105s[1]
Declination+04° 49′ 54.781″[1]
Redshift0.023103[1]
Heliocentric radial velocity6926 ± 2 km/s[1]
Distance350.7 ± 24.6 Mly (107.51 ± 7.54 Mpc)[1]
Apparent magnitude (V)13.5[1]
Characteristics
TypeSA(s)a pec?[1]
Size~162,300 ly (49.77 kpc) (estimated)[1]
Apparent size (V)1.7′ × 0.8′[1]
Other designations
IRAS 11059+0505, 2MASX J11083390+0449545, UGC 6189, MCG +01-29-004, PGC 33760, CGCG 039-010[1]

NGC 3535 is an unbarred spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 7289 ± 25 km/s, which corresponds to a Hubble distance of 107.51 ± 7.54 Mpc (~351 million light-years).[1] It was discovered by German-British astronomer William Herschel on 18 April 1784.

According to the SIMBAD database, NGC 3535 is a radio galaxy.[2]

One supernova has been observed in NGC 3535: SN 2023hrn (type Ia, mag. 18.4) was discovered by ATLAS on 8 May 2023.[3]

See also

References

  1. ^ a b c d e f g h i j k "Results for object NGC 3535". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 29 July 2024.
  2. ^ "NGC 3535". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 14 December 2024.
  3. ^ "SN 2023hrn". Transient Name Server. IAU. Retrieved 14 December 2024.