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Circumstellar envelope

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Part of a star

Acircumstellar envelope (CSE) is a part of astar that has a roughly spherical shape and is not gravitationally bound to the star core. Usually circumstellar envelopes are formed from the densestellar wind, or they are present before the formation of the star.[1] Circumstellar envelopes of old stars (Mira variables andOH/IR stars) eventually evolve intoprotoplanetary nebulae, and circumstellar envelopes ofyoung stellar objects evolve intocircumstellar discs.[2]

Types of circumstellar envelopes

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See also

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References

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  1. ^Leao; Patrick De Laverny; Mekarnia; De Medeiros; Benoit Vandame (2007). "The circumstellar envelope of IRC+10216 from milli-arcsecond to arcmin scales".Astronomy & Astrophysics.455 (1):187–194.arXiv:astro-ph/0703390.Bibcode:2006A&A...455..187L.doi:10.1051/0004-6361:20054577.S2CID 18535333.
  2. ^Leslie Looney; Lee Mundy; Jack Welch (2003). "Envelope Emission in Young Stellar Systems, A Sub-Arcsecond Survey of Circumstellar Structure".The Astrophysical Journal.592 (1):255–265.arXiv:astro-ph/0303640.Bibcode:2003ApJ...592..255L.doi:10.1086/375582.S2CID 15365363.

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