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IC 1266

From Wikipedia, the free encyclopedia
Planetary nebula in the constellation Ara
IC 1266
Nebula
Planetary nebula
IC 1266 imaged byLegacy Surveys
Observation data:J2000.0epoch
Right ascension17h 45m 35.29s
Declination−46° 05′ 23.7″
Distance12,400[1] ly
ConstellationAra
DesignationsIC 1266, Tc 1[2]
See also:Lists of nebulae

IC 1266 (also known asTc 1) is aplanetary nebula located in the southern constellation ofAra. It is a compact emission nebula surrounding a dying star, appearing stellar due to its small angular size and faint gaseous spectrum. Discovered in 1894 by astronomerWilliamina Fleming, IC 1266 lies approximately 12,400light-years from Earth and is best observed from the Southern Hemisphere.[3][4]

Observation and Characteristics

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IC 1266 has an apparent visual magnitude of 11.2 and spans about 0.2 arcminutes in diameter, making it one of the smaller known planetary nebulae.[5] The central star is anO-type starHD 161044, it has aP Cygni type profile.[6]

Spectroscopic and other studies reveal low-excitation lines typical of young planetary nebulae, with abundances of elements and molecules are found like[7] the firstfullerenes in space like C60 and C70[8][9] were discovered in this nebula in 2010 using theSpitzer Space Telescope. These molecules are therefore the largest found in space.[10]

References

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  1. ^Stanghellini, Letizia; Shaw, Richard A.; Villaver, Eva (2008-12-10)."The Magellanic Cloud Calibration of the Galactic Planetary Nebula Distance Scale".The Astrophysical Journal.689 (1):194–202.arXiv:0807.1129.Bibcode:2008ApJ...689..194S.doi:10.1086/592395.ISSN 0004-637X.
  2. ^"IC 1266".simbad.cds.unistra.fr. Retrieved2026-01-25.
  3. ^"IC 1266 - Planetary Nebula in Ara | TheSkyLive".theskylive.com. Retrieved2026-01-25.
  4. ^"Index Catalog Objects: IC 1250 - 1299".cseligman.com. Retrieved2026-01-25.
  5. ^Ford, Dominic."IC1266 (Planetary nebula)".In-The-Sky.org. Retrieved2026-01-25.
  6. ^Feibelman, W. A. (November 1983)."IUE observations of the low-excitation planetary nebula Tc-1".Publications of the Astronomical Society of the Pacific.95: 886.Bibcode:1983PASP...95..886F.doi:10.1086/131266.ISSN 0004-6280.
  7. ^Pottasch, S. R.; Surendiranath, R.; Bernard-Salas, J. (2011-07-01)."Abundances in planetary nebulae: NGC 1535, NGC 6629, He2-108, and Tc1".Astronomy & Astrophysics.531: A23.arXiv:1107.4041.Bibcode:2011A&A...531A..23P.doi:10.1051/0004-6361/201116669.ISSN 0004-6361.
  8. ^Thakur, A.; Lohr, P. J.; Bernal, J. J.; Asaduzzaman, A.; Muralidharan, K.; Zega, T. J.; Ziurys, L. M. (2025-11-01)."A Theoretical Study of Carbon Nanotube Formation: Carriers of the Diffuse Interstellar Bands?".The Astrophysical Journal.993 (1): 18.Bibcode:2025ApJ...993...18T.doi:10.3847/1538-4357/ae06a3.ISSN 0004-637X.
  9. ^Aleman, Isabel; Leal-Ferreira, Marcelo L; Cami, Jan; Akras, Stavros; Ochsendorf, Bram; Wesson, Roger; Morisset, Christophe; Cox, Nick L J; Bernard-Salas, Jeronimo; Paladini, Carlos E; Peeters, Els; Stock, David J; Monteiro, Hektor; Tielens, Alexander G G M (2019-12-01)."Characterization of the planetary nebula Tc 1 based on VLT X-shooter observations".Monthly Notices of the Royal Astronomical Society.490 (2):2475–2494.arXiv:1909.09768.doi:10.1093/mnras/stz2654.ISSN 0035-8711.
  10. ^Cami, Jan; Bernard-Salas, Jeronimo; Peeters, Els; Malek, Sarah Elizabeth (2010-09-03)."Detection of C 60 and C 70 in a Young Planetary Nebula".Science.329 (5996):1180–1182.doi:10.1126/science.1192035.ISSN 0036-8075.
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