RCW 145

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RCW 145
Emission nebula
H II region
RCW 145 (Cropped).png
RCW 145
Observation data: J2000 epoch
Right ascension 18h 02m 18s
Declination −23° 30 56 [1]
Distance2500 [2]   pc
Apparent dimensions (V)1.59° x 1.17°
Constellation Sagittarius
DesignationsNGC 6526, Sh 2-26, Sh 2-28, Gum 74
See also: Lists of nebulae

RCW 145 is an emission nebula in the constellation Sagittarius. RCW 145 contains both Sh 2-26 and Sh 2-28. [3] It is ionized by the supergiant stars LS 4551 and LS 4538. [4] It is possible it is associated with the Trifid nebula. [5]

Contents

Visibility

RCW 145 is often imaged alongside nearby the nebulae of the Lagoon Nebula and Trifid Nebula. The nebula responds well to Hydrogen-alpha filters. It is also easily visible with a Sulfur II filter, however is not very visible in an Oxygen III filter. It is difficult to image with standard RGB. [6]

W 28

In the direction of RCW 145 is also the supernova remnant SNR G006.4-00.1 (W28). W28 lies at a further distance of 1800 to 3300 parsecs. It contains multiple pockets of Maser activity. These pockets are 50-100 milliarcseconds in apparent size. [7] W 28 is visible in most wavelengths, from radio waves to gamma rays. There is some ionization caused by W 28. It was initially thought to be cause by x-ray emissions, however it has since been determined to be cause by cosmic ray emissions. [8]

References

  1. "Sh2-28".
  2. Russeil, D. (2003). "Star-forming complexes and the spiral structure of our Galaxy". Astronomy and Astrophysics. 397: 133. Bibcode:2003A&A...397..133R. doi:10.1051/0004-6361:20021504.
  3. "Sh 2-26".
  4. "Sh 2-28".
  5. Giuliani, A.; et al. (2010). "AGILE detection of GeV γ-ray emission from the SNR W28". Astronomy and Astrophysics. 516. arXiv: 1005.0784 . Bibcode:2010A&A...516L..11G. doi:10.1051/0004-6361/201014256.
  6. "SH2-28 (Sharpless 28)".
  7. "Supernova Remnant W28 · NRAO/AUI Archives".
  8. Phan, V. H. M.; Gabici, S.; Morlino, G.; Terrier, R.; Vink, J.; Krause, J.; Menu, M. (2020). "Constraining the cosmic ray spectrum in the vicinity of the supernova remnant W28: From sub-GeV to multi-TeV energies". Astronomy & Astrophysics. 635: A40. arXiv: 1910.09987 . Bibcode:2020A&A...635A..40P. doi:10.1051/0004-6361/201936927.