Towards an explanation for the 30 Dor (LMC) Honeycomb nebula – the impact of recent observations and spectral analysis

@article{Meaburn2010TowardsAE,
  title={Towards an explanation for the 30 Dor (LMC) Honeycomb nebula – the impact of recent observations and spectral analysis},
  author={J. Meaburn and M. Redman and P. Boumis and Eamonn Harvey Jodrell Bank Centre for Astrophysics and U. O. Manchester and Uk and Centre for Extragalactic Astronomy and S. Physics and National University of Ireland Galway and I. I. O. AstronomyAstrophysics and National Observatory of Athens and Greece.},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2010},
  volume={408},
  pages={1249-1256}
}
  • J. Meaburn, M. Redman, +9 authors Greece.
  • Published 2010
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • The unique Honeycomb nebula, most likely a peculiar supernova remnant, lies in 30 Doradus in the Large Magellanic Cloud (LMC). Due to its proximity to SN1987A, it has been serendipitously and intentionally observed at many wavelengths. Here, an optical spectral analysis of forbidden line ratios is performed in order to compare the Honeycomb high-speed gas with supernova remnants in the Galaxy and the LMC, with Galactic Wolf-Rayet nebulae and with the optical line emission from the interaction… CONTINUE READING
    3 Citations

    Figures from this paper

    References

    SHOWING 1-10 OF 22 REFERENCES
    The Honeycomb supernova remnant
    • 22
    The first broad-band X-ray images and spectra of the 30 Doradus region in the LMC
    • 33
    • PDF
    Ultraviolet interstellar absorption lines in the LMC: Searching for hidden SNRs
    • 34
    Optical Counterpart of the Ultraluminous X-Ray Source IC 342 X-1
    • 37
    • PDF