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Sh 2-307

From Wikipedia, the free encyclopedia
Molecular cloud
Sharpless 2-307
Nebula
Observation data:J2000epoch
Right ascension07h 35m 32s
Declination−18° 45′ 33″[1]
Distance2650 pc
Apparent magnitude (V)15.17
Apparent dimensions (V)6' x 6'[2]
ConstellationPuppis
DesignationsBRAN 50, Gum 7, IRAS 07333-1838, RCW 12, LBN 1051
See also:Lists of nebulae

Sh 2-307 is anebula inPuppis. It contains the potential infrared cluster [DBS2003] 8.[3] It is located in thePerseus Arm.[4] Although appearing small visuallly, longer exposure will reveal the bright area is only the central portion of the nebula, and it is much larger.[5]

References

[edit]
  1. ^"Sh 2-307".
  2. ^"Sharpless (Sh2) - Astrobasics". 13 September 2022.
  3. ^Roman-Lopes, A. (2009)."SOAR-OSIRIS observations of the Sh 2-307 HII region: Triggered star formation beyond the Solar Circle".Monthly Notices of the Royal Astronomical Society.398 (3): 1368.arXiv:0905.3822.Bibcode:2009MNRAS.398.1368R.doi:10.1111/j.1365-2966.2009.15119.x.
  4. ^"Sh 2-307".
  5. ^"CCD Images of the Sharpless Catalog".
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