Home > Science Articles > Peer Reviewed Articles > Empirical mass-loss rates and clumping properties of O-type stars in the Large Magellanic Cloud > Usage statistics
 
 
Empirical mass-loss rates and clumping properties of O-type stars in the Large Magellanic Cloud - Hawcroft, C. et al - published in Astronomy & Astrophysics, 690 issue A126, pp. 18 (2024) - SCART-2025-0092
 
People who viewed this page also viewed:
(254)  STCE Newsletter - Vanlommel, Petra et al - PERIO-2017-0012
(253)  A Comparison of Flare Forecasting Methods. IV. Evaluating Consecutive-Day Forecasting Patterns - Park, Sung-Hong et al - published in The Astrophysical Journal (2020) - SCART-2020-0005
(250)  Automated Detection of Accelerating Solar Eruptions using Parabolic Hough Transform - Patel, Ritesh et al - published in Solar Physics (2020) - SCART-2021-0041
(248)  Gaia Focused Product Release: Asteroid orbital solution. Properties and assessment - Gaia Collaboration et al - published in Astronomy & Astrophysics, 680, pp. A37 (24pp) (2023) - SCART-2024-0008
(248)  TESS Cycle 2 observations of roAp stars with 2-min cadence data - Holdsworth, D. L. et al - published in Monthly Notices of the Royal Astronomical Society, 527 issue 4, pp. 9548--9580 (2024) - SCART-2024-0047


Download history:

Similar records

Space Pole Publications Server :: Search :: Submit :: Personalize :: Help
Powered by Invenio v1.2.1
Maintained by sarah@oma.be