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Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 11/2012, Volume 427, Issue 1, pp. 27 - 49
Abstract We investigate departures from local thermodynamic equilibrium (LTE) in the line formation of Fe for a number of well-studied late-type stars in different evolutionary stages... 
line: formation | line: profiles – radiative transfer | atomic data | stars: abundances | Line: formation | Stars: abundances | Atomic data | Line: profiles - radiative transfer | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Models | Star & galaxy formation | Stars & galaxies | Atmosphere
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2012, Volume 427, Issue 1, pp. 50 - 60
.... The calculations were performed for an extensive grid of 1D marcs models of metal-rich and metal-poor late-type dwarfs and giants... 
stars: fundamental parameters | line: formation | stars: late‐type | atomic data | stars: abundances | Line: formation | Stars: abundances | Stars: late-type | Atomic data | Stars: fundamental parameters | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Stars & galaxies | Spectrum analysis
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 440, Issue 1, pp. 889 - 907
... from disc to spheroid and star formation is quenched rapidly. In contrast, the majority of blue star-forming galaxies have significant discs, and they retain their late-type morphologies as their star formation rates decline very... 
Galaxies: Active | Galaxies: Elliptical and lenticular, cD | Galaxies: Spiral | Galaxies: Evolution | Reservoirs | Ultraviolet radiation | Star & galaxy formation | Morphology | Cosmic rays
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 05/2017, Volume 601, p. A10
S-type stars are late-type giants whose atmospheres are enriched in carbon and s-process elements because of either extrinsic pollution by a binary companion or intrinsic nucleosynthesis and dredge... 
stars: atmospheres | stars: AGB and post-AGB | stars: fundamental parameters | stars: general | stars: late-type | stars: abundances | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics | Astrophysics
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 07/2015, Volume 579, p. A53
Magnesium is an element of significant astrophysical importance, often traced in late-type stars using lines of neutral magnesium, which is expected to be subject to departures from local thermodynamic equilibrium (LTE... 
Line: formation | Stars: abundances | Stars: late-type | Atomic data | Atomic processes | Construction | Inelastic collisions | Stars | Mathematical models | Formations | Magnesium | Collision dynamics | Astronomy | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and astrophysics (Berlin), ISSN 1432-0746, 10/2016, Volume 595, p. A12
Aims. We investigate the photometric modulation induced by magnetic activity cycles and study the relationship between rotation period and activity cycle(s) in late-type (FGKM) stars. Methods... 
stars: low-mass | stars: late-type | stars: activity | techniques: photometric | stars: rotation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Amplitudes | Searching | Modulation | Stars | Sky surveys (astronomy) | Stellar rotation | M stars | Photometry | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 10/2019, Volume 631, p. A80
Manganese (Mn) is a key Fe-group element, commonly employed in stellar population and nucleosynthesis studies to explore the role of SN Ia. We have developed a... 
Physical Sciences | Astronomy & Astrophysics | Science & Technology
Journal Article