Rubidium-rich asymptotic giant branch stars in the Magellanic Clouds

Bibcode
2009iac..talk..112G
García-Hernández, A.; Manchado, A.; Lamber, A. L.; Plez, B.; García-Lario, P.; D'Antona, F.; Lugaro, M.; Karakas, A.; van Raai, M.
Bibliographical reference

IAC Talks, Astronomy and Astrophysics Seminars from the Instituto de Astrofísica de Canarias, p.112

Advertised on:
11
2009
Number of authors
9
IAC number of authors
1
Citations
0
Refereed citations
0
Description
Not Available
Type
Non-refereed

It may interest you

  • Non-refereed
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Advertised on:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Citations
    0
  • Non-refereed
    ANDES, the high-resolution spectrograph for the ELT: design of the adaptive optics system
    ANDES,the high resolution spectrograph for the ELT, will work both in seeing limited mode and with Adaptive Optics (AO) correction. ANDES-SCAO is a single conjugated AO system working with natural guide stars, feeding the IFU coupled to the YJH spectrograph. The main science goal of the ANDES AO mode is the characterization of the exo-planet
    Pinna, Enrico et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13097E..4WP
    Citations
    0