The VLT-FLAMES Tarantula survey

Bibcode
2011IAUS..272..296L
DOI
10.1017/S1743921311010647
Lennon, Daniel J.; Evans, Christopher J.; Bastian, Nate; Beletsky, Yuri; Brott, Ines; Cantiello, Matteo; Carraro, Giovanni; Clark, J. Simon; Crowther, Paul A.; de Koter, Alex; de Mink, Selma E.; Dufton, Philip L.; Dunstall, Paul; Gieles, Mark; Gräfener, Goetz; Hénault-Brunet, Vincent; Herrero, Artemio; Howarth, Ian D.; Langer, Norbert; Maíz Apellániz, Jesús; Markova, Nevena; Najarro, F. Paco; Puls, Joachim; Sana, Hugues; Simón-Díaz, Sergio; Smartt, Stephen J.; Stroud, Vanessa E.; Taylor, William D.; van Loon, Jacco T.; Vink, Jorick S.; Walborn, Nolan R.
Bibliographical reference

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU Symposium, Volume 272, p. 296-297

Advertised on:
7
2011
Number of authors
31
IAC number of authors
0
Citations
3
Refereed citations
1
Description
The Tarantula Survey is an ESO Large Programme which has obtained multi-epoch spectroscopy of over 1,000 massive stars in the 30 Doradus region of the Large Magellanic Cloud. The assembled consortium will exploit these data to address a range of fundamental questions in both stellar and cluster evolution.
Type
Non-refereed

It may interest you

  • Non-refereed
    Workshop summary: Kaons@CERN 2023

    Kaon physics is at a turning point - while the rare-kaon experiments NA62 and KOTO are in full swing, the end of their lifetime is approaching and the future experimental landscape needs to be defined. With HIKE, KOTO-II and LHCb-Phase-II on the table and under scrutiny, it is a very good moment in time to take stock and contemplate about the

    Anzivino, G. et al.

    Advertised on:

    4
    2024
    Bibcode
    2024EPJC...84..377A
    Citations
    0
  • Non-refereed
    First light and results for atmospheric characterization with The Near Infra-Red Planet Searcher (NIRPS)

    NIRPS is a new fiber-fed high spectral resolution (~80k) spectrograph assisted by adaptive optics installed on the 3.6m telescope of ESO at LaSilla, Chile. Operated simultaneously with HARPS, NIRPS covers the Y, J, and H bands. The commissioning phase demonstrated high stability for time-series observations along precise radial velocities reaching

    Allart, Romain et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ESS.....562419A
    Citations
    0
  • Non-refereed
    Nodal Precession of a Hot Jupiter Transiting the Edge of a Late A-Type Star TOI-1518

    TOI-1518b, a hot Jupiter around a late A-type star, is one of the few planetary systems that transit the edge of the stellar surface (the impact parameter b~0.9) among hot Jupiters around hot stars (Cabot et al. 2021). The host star's high rotation speed (Vsini s~85 km s -1) and the planet's nearly polar orbit (λ~120 deg) may cause a nodal

    Watanabe, Noriharu et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ESS.....561705W
    Citations
    0
Go back