Results 281 to 290 of about 207,560 (312)
Exo-Geoscience Perspectives Beyond Habitability. [PDF]
Spohn T +7 more
europepmc +1 more source
Pattern functions of the Astrometric Gravitational Wave Antenna. [PDF]
Santucci F, Crosta M, Lattanzi MG.
europepmc +1 more source
Determination of the mass distribution of the first stars from the 21-cm signal. [PDF]
Gessey-Jones T +8 more
europepmc +1 more source
Single-port <i>versus</i> multiport robotic surgery in head and neck procedures: a systematic review and meta-analysis of surgical parameters. [PDF]
Mahfoz TB.
europepmc +1 more source
Relationship Between Anemia and Oral Lichen Planus: New Therapeutic Perspectives Based on Anemia Management-A Systematic Review and Meta-Analysis. [PDF]
Egido-Moreno S +5 more
europepmc +1 more source
Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]
Cang T +13 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Monthly notices of the Royal Astronomical Society, 2023
Classical Be stars are fast rotating, near main sequence B-type stars. The rotation and the presence of circumstellar discs profoundly modify the observables of active Be stars.
A. Rubio +16 more
semanticscholar +1 more source
Classical Be stars are fast rotating, near main sequence B-type stars. The rotation and the presence of circumstellar discs profoundly modify the observables of active Be stars.
A. Rubio +16 more
semanticscholar +1 more source
Fundamental parameters for 222 B-type stars for the X-shooter Spectral Library
Proceedings of the International Astronomical Union, 2022We use the MIDE3700 code to find effective temperatures (Teff) and surface gravities (log g) via the Barbier Chalonge Divan (BCD) method for 222 B-type stars in the ESO archive in preparation for their inclusion as an extension to the X-shooter Spectral ...
C. Larkin +3 more
semanticscholar +1 more source
The Fundamental Parameters of Massive Stars
AIP Conference Proceedings, 2009We analyzed far‐UV (FUSE), UV (HST, IUE) and optical spectra of hot massive stars in the Milky Way with non‐LTE, line‐blanketed models with sphericity and expanding winds. We were able to reconcile previously discrepant diagnostics from Hα to highly ionized transitions (e.g.
Luciana Bianchi +6 more
openaire +1 more source

