Mapping the kinematics and chemistry of the Solar neighborhood with a 61cm telescope

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no. 3

A. Milani - P. Valisa - U. Munari

Detaily:

Rok, strany: 2014, 537 - 538

Kľúčové slová:

Galaxy: kinematics and dynamics, Galaxy: solar neighborhood

URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2014/Vol_43/No_3/pp537-538_abstract.html

Full text

O článku:

The 61cm Varese telescope and its Multi Mode Spectrograph operated in the Echelle mode is used to observe nearby Red Clump stars in the Solar neighborhood, with more distant ones being targeted by Asiago 1.22m and 1.82m telescopes. So far high resolution, high S/N spectra of 260 program RC stars have been obtained (85 on a 2^nd epoch) providing radial velocities accurate to 0.7 km/s, T_eff to 56 K, logg to 0.21 dex, and [M/H] to 0.11 dex.

Ako citovať:

ISO 690:

Milani, A., Valisa, P., Munari, U. 2014. Mapping the kinematics and chemistry of the Solar neighborhood with a 61cm telescope. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no.3, pp. 537-538. 1335-1842.

APA:

Milani, A., Valisa, P., Munari, U. (2014). Mapping the kinematics and chemistry of the Solar neighborhood with a 61cm telescope. Contributions of the Astronomical Observatory Skalnaté Pleso, 43(3), 537-538. 1335-1842.