Browsing by Subject "Stellar winds"

Browsing by Subject "Stellar winds"

Sort by: Order: Results:

  • Thumbnail
    A study of molecular gas associated with the HH24 optical jets 
    Ma, Lifang (Halifax, N.S. : Saint Mary's University, 1994)
    The HH24 complex have been mapped in 12CO J=3-2 emission at 14" resolution, using the 15m James Clerk Maxwell Telescope (JCMT) on Manna Kea, Hawaii. The map in 12CO J=3-2 shows complicated morphology ...

  • Thumbnail
    The evolution of very massive stars 
    Bever, J. Van; Belkus, H.; Vanbeveren, D. (American Astronomical Society, 2007-04)
    Core collapse of dense massive star clusters is unavoidable, and this leads to the formation of massive objects, with masses of up to 1000 M[circled dot] and even larger. When these objects become stars, stellar wind mass ...

  • Thumbnail
    MOST finds no coherent oscillations in the hot carbon-rich Wolf-Rayet star HD 165763 (WR 111) 
    Guenther, David B.; Moffat, A. F. J.; Marchenko, S. V.; Zhilyaev, B. E.; Rowe, J. F.; Muntean, V.; Chene, A.-N.; Matthews, J. M.; Kuschnig, R.; Rucinski, S. M. (American Astronomical SocietyIOP Publishing, 2008-05-20)
    We have photometrically monitored the V = 8 mag Galactic Population I WC5 star WR 111 for 3 weeks nonstop using the MOST microsatellite. Each of the ∼27,000 data points has a precision of ∼3 mmag. We find no coherent Fourier ...

  • Thumbnail
    Testing the ergodicity of star formation within galaxies 
    Smith, Fraser M. (Halifax, N.S. : Saint Mary's University, 2023-08-11)
    Part of our understanding of how galaxies evolve is based on individual evolutions inferred from population trends. In its strictest form, this approach implicitly assumes that the star formation properties of galaxies ...

  • Thumbnail
    WR 110: a single Wolf–Rayet star with corotating interaction regions in its wind? 
    Chene, A.-N.; Moffat, A. F .J.; Cameron, Chris; Fahed, R.; Gamen, R. C.; Lefevre, L.; Rowe, J. F.; St.-Louis, N.; Muntean, V.; De La Chevrotiere, A.; Guenther, David B. (American Astronomical Society, 2011-07-01)
    A 30 day contiguous photometric run with the Microvariability and Oscillations of STars (MOST) satellite on the WN5-6b star WR 110 (HD 165688) reveals a fundamental periodicity of P = 4.08 ± 0.55 days along with a number ...