output
19932026
most citedThe Gaia mission

7.1k citations

Showing 2013 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2013★ 1 cited

Relative frequencies of supernovae versus properties of spiral hosts

A. A. Hakobyan, T. A. Nazaryan, V. Zh. Adibekyan +8

In this work, we present an analysis of SNe number ratios in spiral galaxies with different morphological subtypes, luminosities, sSFR, and metallicities, to provide important info…

astro-ph.GA2013★ 46 cited

What will blue compact dwarf galaxies evolve into?

Hagen T. Meyer, Thorsten Lisker, Joachim Janz +1

We present and analyse the photometric properties of a nearly complete sample of blue compact dwarf (BCD) and irregular galaxies in the Virgo cluster from multi-band SDSS images. O…

astro-ph.GA2013★ 28 cited

Limits on the spatial variations of the electron-to-proton mass ratio in the Galactic plane

S. A. Levshakov, D. Reimers, C. Henkel +4

Aims. To validate the Einstein equivalence principle (local position invariance) by limiting the fractional changes in the electron-to-proton mass ratio, mu = m_e/m_p, measured in…

astro-ph.GA2013★ 314 cited

Gaia FGK Benchmark Stars - Metallicity

Paula Jofre, U. Heiter, C. Soubiran +22

To calibrate automatic pipelines that determine atmospheric parameters of stars, one needs a sample of stars -- ``benchmark stars'' -- with well defined parameters to be used as a…

astro-ph.GA2013★ 161 cited

Kinematics and chemical properties of the Galactic stellar populations. The HARPS FGK dwarfs sample

V. Zh. Adibekyan, P. Figueira, N. C. Santos +7

(Abridged) We analyze chemical and kinematical properties of about 850 FGK solar neighborhood long-lived dwarfs observed with the HARPS high-resolution spectrograph. The stars in t…

astro-ph.GA2013★ 126 cited

A candidate circumbinary Keplerian disk in G35.20-0.74 N: A study with ALMA

A. Sanchez-Monge, R. Cesaroni, M. T. Beltran +13

We report on ALMA observations of continuum and molecular line emission with 0.4" resolution towards the high-mass star forming region G35.20-0.74 N. Two dense cores are detected i…