NGC 3987

NGC 3987
NGC 3987 imaged by SDSS
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 57m 20.9684s[1]
Declination+25° 11′ 42.874″[1]
Redshift0.015018±0.000017[1]
Heliocentric radial velocity4,502±5 km/s[1]
Distance196.49 ± 4.62 Mly (60.243 ± 1.415 Mpc)[1]
Group or clusterNGC 3987 Group (LGG 261), Holm 308
Apparent magnitude (V)12.9B[1]
Characteristics
TypeSb[1]
Size~179,000 ly (54.88 kpc) (estimated)[1]
Apparent size (V)2.2′ × 0.4′[1]
Other designations
HOLM 308C, IRAS 11547+2528, 2MASX J11572090+2511436, UGC 6928, MCG +04-28-099, PGC 37591, CGCG 127-110[1]

NGC 3987 is a spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 4,810±10 km/s, which corresponds to a Hubble distance of 231.4 ± 16.2 Mly (70.94 ± 4.98 Mpc).[1] However, 23 non-redshift measurements give a closer distance of 196.49 ± 4.62 Mly (60.243 ± 1.415 Mpc).[2] It was discovered by German-British astronomer William Herschel on 6 April 1785.[3][4]

NGC 3987 has an active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.[5] In addition, it is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[1]

Holm 308 and NGC 3987 group

NGC 3987, NGC 3989, NGC 3993 and NGC 3997 are listed together as Holm 308 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.[6]

However, according to A. M. Garcia, NGC 3987 is the largest galaxy in a group that bears its name. The NGC 3987 group (also known as LGG 261) is thought to have at least five galaxies, including NGC 4000, NGC 4005, NGC 4018, and NGC 4022.[7]

Supernovae

Two supernovae have been observed in NGC 3987:

  • SN 2001V (Type Ia, mag. 16) was discovered by P. Berlind on 19 February 2001.[8][9] Later analysis concluded that this supernova was overluminous, and its spectral features indicate it might be a SN 1999aa-like object.[10]
  • SN 2025msx (Type Ic-BL, mag. 18.914) was discovered by ATLAS on 1 June 2025.[11]

See also

References

  1. ^ a b c d e f g h i j k l "Results for object NGC 3987". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 14 July 2025.
  2. ^ "Distance Results for NGC 3987". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 14 July 2025.
  3. ^ Herschel, W. (1786). "Catalogue of One Thousand New Nebulae and Clusters of Stars" (PDF). Philosophical Transactions of the Royal Society of London. 76: 457–499. Bibcode:1786RSPT...76..457H. doi:10.1098/rstl.1786.0027.
  4. ^ Seligman, Courtney. "New General Catalogue Objects: NGC 3987". Celestial Atlas. Retrieved 13 July 2025.
  5. ^ "NGC 3987". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 14 July 2025.
  6. ^ Holmberg, Erik (1937). "A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems". Annals of the Observatory of Lund. 6: 1. Bibcode:1937AnLun...6....1H.
  7. ^ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
  8. ^ Jha, S.; Matheson, T.; Challis, P.; Kirshner, R.; Berlind, P. (2001). "Supernova 2001V in NGC 3987". International Astronomical Union Circular (7585): 1. Bibcode:2001IAUC.7585....1J.
  9. ^ "SN 2001V". Transient Name Server. IAU. Retrieved 14 July 2025.
  10. ^ Vinkó, J.; Bíró, I. B.; Csák, B.; Csizmadia, Sz.; Derekas, A.; Furész, G.; Heiner, Z.; Sárneczky, K.; Sipocz, B.; Szabó, Gy.; Szabó, R.; Sziládi, K.; Szatmáry, K. (2003). "The Type Ia Supernova 2001V in NGC 3987". Astronomy and Astrophysics. 397: 115. arXiv:astro-ph/0210186. Bibcode:2003A&A...397..115V. doi:10.1051/0004-6361:20021469.
  11. ^ "SN 2025msx". Transient Name Server. IAU. Retrieved 14 July 2025.


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