Giants in the Local Region
By R. E. Luck, U. Heiter. 2007
164 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/41094ac38c30fd0ed24d3bad82659633f1ed6e15
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- C. Allende Prieto
- I. Ramírez
- I. Minchev
- Timothy C. Beers
- Martin Asplund
- Jo Bovy
- Hans-Walter Rix
- C. Chiappini
In Instrumentation
- I. Minchev
- Timothy C. Beers
- C. Allende Prieto
- C. Chiappini
- M. Koleva
- I. Ramírez
- Hans-Walter Rix
- Y. S. Lee
Citations in the corpus
- THE METALLICITY DISTRIBUTION FUNCTIONS OF SEGUE G AND K DWARFS: CONSTRAINTS FOR DISK CHEMICAL EVOLUTION AND FORMATION (2011, background): “…spectroscopic analyses of these low-luminosity targets were limited to hundreds of stars along individual lines of sight (Wyse & Gilmore 1995; Favata et al. 1997; Fuhrmann 1998, 2004, 2008, 2011; Allende Prieto et al. 2004; Luck & Heiter 2005, 2006, 2007; Arnadottir et al. 2009; Katz et al. 2011).”
- Stellar Parameters and Elemental Abundances of Late-G Giants (2008, methodology): “K giants, as well as to the three latest studies available (da Silva et al. 2006, Luck & Heiter 2007, and Hekker & Meléndez 2007).”
- The PASTEL catalogue of stellar parameters (2010, unknown): “– Hekker= Hekker & Meléndez (2007), 366 stars – Luck= Luck & Heiter (2006, 2007), 222 stars – McWilliam =McWilliam (1990), 671 stars – Mishenina = Mishenina & Kovtyukh (2001); – Ramı́rez= Ramı́rez et al. (2007), 523 stars – Valenti= Valenti & Fischer (2005) , 1040 stars studies can be considered…”
- OXYGEN ABUNDANCES IN NEARBY FGK STARS AND THE GALACTIC CHEMICAL EVOLUTION OF THE LOCAL DISK AND HALO (2013, background): “For example, in their extensive abundance analysis of stars in the local region, Luck & Heiter (2006, 2007) find that their oxygen abundance trends for dwarf and giant stars are equivalent.”
- Chemical similarities between Galactic bulge and local thick disk red giants: O, Na, Mg, Al, Si, Ca, and Ti (2010, background): “analysis of∼180 clump giants by Mishenina et al. (2006), the study of∼300 nearby giants by Luck & Heiter (2007), the survey of ∼380 giants by Hekker & Meléndez (2007), and the analysis of ∼320 giants by Takeda et al. (2008).”
- SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs - I. New atmospheric parameters and masses for 48 stars with planets (2013, methodology): “For the remaining stars, values were compiled from the literature, both from the discovery papers or from other compilations/catalogs (e.g. Luck & Heiter 2007; Soubiran et al. 2010).”
- Precise radial velocities of giant stars. III. Spectroscopic stellar parameters (2007, methodology): “Indeed, in a large study of several hundreds of giantsand dwarfs, Luck & Heiter (2007) show that the abundances of Fe, Mn and Ba in giants may be affected by systematic uncertainties when compared with dwarf stars.”
- Coudé-feed stellar spectral library – atmospheric parameters (2010, background): “They found their results to be consistent with Luck & Heiter (2007).”
- Gaia FGK benchmark stars: Effective temperatures and surface gravities (2015, methodology): “The parallax-log g value by Luck & Heiter (2007) is based on isochrones from a previous version of the Padova models (Bertelli et al. 1994).”