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Pre‐oxygenation using high‐flow nasal oxygen vs. tight facemask during rapid sequence induction
Anaesthesia, 2021Sabine Nabecker, L Theiler
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Luminous pre-main sequence stars in the LMC?
Astronomy & Astrophysics, 1999We report the serendipitous discovery of seven luminous irregular variables in the LMC by the EROS project. The stars have V similar or equal to 15(m) to 17(m), (B(E) - R(E)) similar or equal to 0(m), and vary by about 0.4(m) on timescales of 10 to 40 days.
Lamers, HJGLM, Beaulieu, JP
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Accretion onto Pre-Main-Sequence Stars
Annual Review of Astronomy and Astrophysics, 2016Lee Hartmann +2 more
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Proper Motions of Pre-Main Sequence Stars
2014The kinematic study of young stars is an important tool to discuss the early stages of star formation. In this context, proper motions allow us to detect moving group structures of young stars to which they belong. Individual distances to moving group members can be inferred from proper motion and radial velocity data using the convergent point ...
Ferreira, A. C. S., +5 more
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