The "Papillon" nebula: a compact H II blob in the LMC resolved by HST *
M. Heydari-Malayeri 1,
M.R. Rosa ** 2,
V. Charmandaris 1,
L. Deharveng 3 and
H. Zinnecker 4
Received 26 April 1999 / Accepted 12 July 1999
We present high spatial resolution HST imaging of the LMC compact H II region N159-5. This high excitation blob is revealed to be a "papillon" or butterfly-shaped ionized nebula with the "wings" separated by (0.6 pc). Two subarcsecond features resembling a "smoke ring" and a "globule" are detected in the wings, the origin of which is briefly discussed. N159-5 may represent a new type of H II region in the Magellanic Clouds overlooked so far because of insufficient spatial resolution. Our images also show a strikingly turbulent medium around the Papillon in the giant H II region N 159, which manifests itself by a large number of subarcsecond filaments, arcs, ridges, and fronts carved in the ionized gas by the stellar winds from massive stars in the N 159 complex.
Key words: galaxies: Magellanic Clouds ISM: kinematics and dynamics ISM: individual objects: N 159-5 ISM: H ii regions ISM: dust, extinction stars: early-type
* Based on observations with the NASA/ESA Hubble Space Telescope obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.
Send offprint requests to: M. Heydari-Malayeri (firstname.lastname@example.org)
© European Southern Observatory (ESO) 1999
Online publication: December 2, 1999