Illustration par défaut

A BUTTERFLY-SHAPED "PAPILLON" NEBULA YIELDS SECRETS OF MASSIVE STAR BIRTH

1er septembre 1999 A BUTTERFLY-SHAPED "PAPILLON" NEBULA YIELDS SECRETS OF MASSIVE STAR BIRTH

A rare type of compact ionized "blob" is resolved for the first time to be a butterfly-shaped or "Papillon" (French for "butterfly") nebula, buried in the center of the maelstrom of glowing gases and dark dust. The unprecedented details of the structure of the Papillon, itself less
than 2 light-years in size (about 2 arcseconds in the sky), are seen in the inset.

A possible explanation of this bipolar shape is the outflow of gas from massive stars (over 10 times the mass of our sun) hidden in the central absorption zone. Such stars are so hot that their radiation pressure halts the infall of gas and directs it away from the stars in two opposite directions. Presumably, a dense equatorial disk formed by matter still trying to fall in onto the stars focuses the outstreaming matter into the bipolar directions.
This observation is part of a search for young massive stars in the LMC. Rare are the cases where we can see massive stars so early after their birth.

The red in this true-color image is from the emission of hydrogen and the yellow from high excitation ionized oxygen. The picture was taken on September 5, 1998 with the Wide Field Planetary Camera 2.

The Hubble observations of the Papillon nebula were conducted by the

European astronomers

  • Mohammad Heydari-Malayeri-(DEMIRM / CNRS, Observatoire de Paris) and co-investigators :
  • -* Michael Rosa (Space Telescope European Coordinating Facility, Observatoire Européen Austral, Allemagne),
  • Vassilis Charmandaris (DEMIRM / CNRS, Observatoire de Paris),
  • Lise Deharveng (Observatoire de Marseille, France),
  • Hans Zinnecker (Astrophysical Institute, Potsdam, Allemagne).

Their work is submitted for publication in the European journal Astronomy and Astrophysics.