From Wikipedia, the free encyclopedia
L183
Molecular cloud
Observation data: J2000 epoch
Right ascension15h 54m 12.2s [1]
Declination−02° 49′ 42″ [1]
Distance360[ citation needed]  ly
Apparent diameter75 [1]
Constellation Serpens
DesignationsLDN 134N
See also: Lists of nebulae

L183 or L134N is a much-studied pre-stellar core in the constellation Serpens Cauda 360 light-years away. This massive accumulation of gas and dust was the interstellar object in which the phenomenon of coreshine was first investigated by astronomers and produced a new means of probing its previously opaque core. [2] [3]

References

  1. ^ a b c "LDN 183". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 September 2017.
  2. ^ L183 (L134N) Revisited - L. Pagani, A. Bacmann et al.
  3. ^ Charlotte Vastel, T.G Phillips, P Caselli, C Ceccarelli and L Pagani Deuterium enhancement in pre-stellar cores


From Wikipedia, the free encyclopedia
L183
Molecular cloud
Observation data: J2000 epoch
Right ascension15h 54m 12.2s [1]
Declination−02° 49′ 42″ [1]
Distance360[ citation needed]  ly
Apparent diameter75 [1]
Constellation Serpens
DesignationsLDN 134N
See also: Lists of nebulae

L183 or L134N is a much-studied pre-stellar core in the constellation Serpens Cauda 360 light-years away. This massive accumulation of gas and dust was the interstellar object in which the phenomenon of coreshine was first investigated by astronomers and produced a new means of probing its previously opaque core. [2] [3]

References

  1. ^ a b c "LDN 183". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 September 2017.
  2. ^ L183 (L134N) Revisited - L. Pagani, A. Bacmann et al.
  3. ^ Charlotte Vastel, T.G Phillips, P Caselli, C Ceccarelli and L Pagani Deuterium enhancement in pre-stellar cores



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