NGC 3435

Today, we will delve into the exciting world of NGC 3435, a topic that has captured the attention of millions of people around the world. From its origins to its impact on today's society, NGC 3435 has played a fundamental role in people's daily lives and has generated endless debates and controversies. Through this article, we will explore the many facets of NGC 3435, examining its influence on different aspects of modern life and analyzing its evolution over time. Immerse yourself in this journey of discovery and join us in exploring NGC 3435 in all its dimensions.

NGC 3435
NGC 3435
NGC 3435
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension10h 54m 48.3299s[1]
Declination+61° 17′ 23.483″[1]
Redshift5 181 ± 2 km/s
Apparent magnitude (V)13.2
Characteristics
Typebarred spiral galaxy
Apparent size (V)1.8′ × 1.2′
Other designations
PGC 32786, UGC 6025, MCG 10-16-22, CGCG 291.12, IRAS10517+61322

NGC 3435 is a barred spiral galaxy located about 235 million light-years from the Milky Way, and is about 125 000 light-years across. It can be found in the constellation Ursa Major. It was discovered on 9 April 1793 by astronomer William Herschel.[2]

The galaxy has the surface brightness equal to 14.04 mag/Minute and second of arcam², which classifiers it as low surface brightness galaxy (LSB).[3]

Supernova

On 29 March 1999, in the galaxy was observed the type Ia supernova, designated as SN 1999bh.[4] It was discovered by W. Li, as part of the Lick Observatory Supernova Search (LOSS) program by the Lick Observatory.[5][6]

References

  1. ^ a b "NGC 3435". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2024-10-26.
  2. ^ Courtney Seligman: NGC 3435, Celestial Atlas.
  3. ^ Les données de «Revised NGC and IC Catalog by Wolfgang Steinicke» sur le site ProfWeb, NGC 3400 à 3499
  4. ^ "List of Supernovae". cbat.eps.harvard.edu.
  5. ^ IAUC 7135: 1999bg; 1999bh; C/1995 O1
  6. ^ Bright Supernovae - 1999[permanent dead link]