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pro vyhledávání: '"Klaus Fuhrmann"'
Autor:
Rolf Chini, Klaus Fuhrmann
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 501:4903-4916
We report on the progress of our survey on ancient solar-type stars down to main-sequence effective temperatures Teff ≥ 5300 K and within 42 pc of the Sun. High signal-to-noise, high-resolution spectroscopy is presented for a second major subset of
Autor:
Klaus Fuhrmann, Rolf Chini
Publikováno v:
Research Notes of the AAS. 6:14
The bright star γ Psc is among the nearest Population II giants located in the red clump region. Here we demonstrate that γ Psc is actually a core-helium burning horizontal branch star. As such, the τ ≃ 12 Gyr old γ Psc is found to be slightly
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 471:3768-3774
We report an intrinsically precise relation of the barium-to-iron enrichment as a function of age for a local, volume-complete (N = 30) sample of ancient Population II (tau >= 12 Gyr) and intermediate-disc stars (tau similar or equal to 10 Gyr), whic
Autor:
Rolf Chini, Klaus Fuhrmann
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 471:1888-1891
Autor:
Monika Thym, Sylvia Braasch, Davor Stubican, Ulrich Körner, Klaus Fuhrmann, Florian Schäffler, Gudrun Kolb, Manuela Bolz
Publikováno v:
Suchttherapie. 19:90-98
ZusammenfassungZiel des Projekts war es, den Anteil von Klientel mit Doppelbelastung (altersassoziierte Problemlagen in der Suchthilfe, Sucht in der Altenhilfe) zu ermitteln sowie die Bedarfe von Mitarbeitenden beider Hilfesysteme zu eruieren.Hierzu
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 464:2610-2621
We present a study of the local stellar populations from a volume-complete all-sky survey of the about 500 bright stars with distances less than 25 pc and down to main-sequence effective temperatures T-eff >= 5300 K. The sample is dominated by a 93 p
Autor:
N. Niedworok, Klaus Fuhrmann, Michael Ramolla, Klaus W. Hodapp, F. Pozo Nuñez, L. Kaderhandt, Rolf Chini
Publikováno v:
Astronomische Nachrichten. 337:621-626
Gliese 29 is a 7 to 8 Gyr old, southern Population I turnoff star with a large proper motion of 1″/yr. Using recent direct imaging observations with the 0.8 m Infrared Imaging System (IRIS) of the Universitatssternwarte Bochum near Cerro Armazones
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 459:1682-1686
We report the discovery of a tertiary component to the prominent and nearby (d = 14 pc) visual binary alpha Fornacis. The new invisible component is part of a 4-d short-period Ba-Bb subsystem, whose K-type alpha For Ba primary shows a striking [Ba/Fe
Autor:
Klaus Fuhrmann, Rolf Chini
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
Autor:
Rolf Chini, Klaus Fuhrmann
Publikováno v:
Research Notes of the AAS. 3:142