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NGC 1035

From Wikipedia, the free encyclopedia
Spiral galaxy located on the Cetus constellation
NGC 1035
Image of NGC 1035 obtained from the Sloan Digital Sky Survey
Observation data
ConstellationCetus
Right ascension02h 40m 44s
Declination-08° 01’ 28”
Absolute magnitude (B)12.89
Surface brightness22.36
magnitude (J)10.12
magnitude (H)9.42
magnitude (K)9.13
Characteristics
TypeSpiral galaxy

NGC 1035 is aspiral galaxy located in theConstellation ofCetus. It is situated close to thecelestial equator making it at least partially visible on both sides of thehemisphere during certain times of the year.[1]

The neighboring galaxyNGC 1052-DF4 shows signs of beingtidally disrupted and is missing most of itsdark matter. The cause for this missing dark matter is from this galaxy stripping the dark matter from NGC 1052-DF4 and is now stripping apart the galaxy itself. Only thecentral regions of NGC 1052-DF4 remains unaffected.[2]

Supernova

[edit]

SN 1990E is aType ll supernova that occurred in thisgalaxy.[3]

References

[edit]
  1. ^"NGC 1035 - Spiral Galaxy in Cetus | TheSkyLive".theskylive.com. Retrieved2025-06-14.
  2. ^information@eso.org."New Hubble Data Explains Missing Dark Matter".www.esahubble.org. Retrieved2025-06-14.
  3. ^Schmidt, Brian P.; Kirshner, Robert P.; Schild, Rudy; Leibundgut, Bruno; Jeffery, David; Willner, S. P.; Peletier, Reynier; Zabludoff, Ann I.; Phillips, Mark M.; Suntzeff, Nicholas B.; Hamuy, Mario; Wells, Lisa A.; Smith, R. Chris; Baldwin, Jack A.; Weller, W. G. (June 1993)."Photometric and Spectroscopic Observations of SN 1990E in NGC 1035 Observational Constraints for Models of Type II Supernovae".The Astronomical Journal.105: 2236.doi:10.1086/116602.ISSN 0004-6256.
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