The VLT-FLAMES Survey of Massive Stars

Bibcode
2010ASPC..425...29L
Lennon, D. J.; Evans, C.; Hunter, I.; Trundle, C.; Smartt, S.; Dufton, P.; Ryans, R.; Langer, N.; Brott, I.; de Koter, A.; Mokiem, R.; Puls, J.; Herrero, A.; Howarth, I.
Bibliographical reference

Hot and Cool: Bridging Gaps in Massive Star Evolution ASP Conference Series Vol. 425, Proceedings of a Workshop held at the California Institute of Technology, Pasadena, California, 10-12 November 2008. Edited by Claus Lietherer, Philip Bennett, Pat Morris, Jacco van Loon. San Francisco: Astronomical Society of the Pacific, 2010., p.29

Advertised on:
6
2010
Number of authors
14
IAC number of authors
0
Citations
0
Refereed citations
0
Description
The VLT-FLAMES Survey of Massive Stars in the Galaxy, the Large and Small Magellanic Clouds was an ESO Large Program (P.I. S. Smartt) aimed at understanding rotational mixing and stellar mass loss in environments of differing metallicity (Z). The overarching goal is to better understand massive star evolution.
Type
Non-refereed

It may interest you

  • Non-refereed
    Co-phasing the distributed aperture of a Fizeau interferometer via photonic lanterns and machine learning
    The advantage of large optical telescopes from the ground for high-contrast direct imaging relies on achieving exquisite control of the incident optical wavefront. Since the exoplanet problem almost always has a bright star within a small field of view there are usually ample photons for measuring the atmospheric and telescopedistorted wavefront. A
    Padrón-Brito, Auxiliadora et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..25P
    Citations
    0
  • Non-refereed
    Unveiling Chiron, an odd ice ball, with Webb: Ice and Gas Phases Revealed
    We present unprecedented findings on (2060) Chiron using James Webb Space Telescope (JWST) NIRSpec imaging and spectroscopy from cycle 1 GTO program 1273. Our study (Pinilla-Alonso et al. 2024 A&A Letter) marks the first detection of carbon dioxide (CO 2) and methane (CH 4) active outgassing and coma emission at heliocentric distances of ~18 au
    Pinilla-Alonso, Noemí et al.

    Advertised on:

    10
    2024
    Bibcode
    2024DPS....5640508P
    Citations
    0
  • Non-refereed
    Conceptual optical design of the infrared integral field spectropolarimeter for the European Solar Telescope
    The European Solar Telescope (EST), with its primary mirror of 4.2 diameter, will be the largest solar telescope available in Europe. EST will offer Integral Field Spectropolarimetry (IFS) by incorporating the EST spectropolariMeter Based on slicEr-mirrors for the near-infraRed (EMBER). This instrument is a high-resolution spectropolarimeter that
    Regalado Olivares, S. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13100E..5FR
    Citations
    0