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1,266 results on '"Molaro, P"'

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151. An extremely primitive halo star

152. A primordial star in the heart of the Lion

153. X-Shooter GTO: Chemical analysis of a sample of EMP candidates

154. First measurement of Mg isotope abundances at high redshifts and accurate estimate of Delta alpha/alpha

155. Extremely metal-poor stars in SDSS fields

156. First stars XIII. Two extremely metal-poor RR Lyrae stars?

157. Optical-NIR spectra of quasars close to reionization (z~ 6)

158. First Stars XIV. Sulfur abundances in extremely metal-poor (EMP) stars

159. Searching for Chameleon-like Scalar Fields

160. Robust limit on a varying proton-to-electron mass ratio from a single H2 system

161. Searching for chameleon-like scalar fields with the ammonia method. II. Mapping of cold molecular cores in NH3 and HC3N lines

162. Ammonia as a Tracer of Fundamental Constants

163. Searching for spatial variations of alpha^2/mu in the Milky Way

164. The metal-poor end of the Spite plateau. 1: Stellar parameters, metallicities and lithium abundances

165. Spatial and temporal variations of fundamental constants

166. Searching for chameleon-like scalar fields with the ammonia method

167. Cosmological observations to shed light on possible variations - expectations, limitations and status quo

168. Calibration issues in estimating variability of the fine structure constant (alpha) with cosmic time

169. Metal-rich absorbers at high redshifts: abundance patterns

170. The mystery of the telescopes in Jan Brueghel the Elder's paintings

171. On the telescopes in the paintings of J. Brueghel the Elder

172. Stringent bounds to spatial variations of the electron-to-proton mass ratio in the Milky Way

173. First stars XII. Abundances in extremely metal-poor turnoff stars,and comparison with the giants

174. Revisiting the classics: On the evolutionary origin of the ‘Fe II’ and ‘He/N’ spectral classes of novae

175. A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO

176. On spatial variations of the electron-to-proton mass ratio in the Milky Way

177. From Espresso to Codex

178. Cosmic dynamics in the era of Extremely Large Telescopes

179. Quasar spectral energy distribution in EUV restored from associated absorbers: indications to the HeII opacity of the quasar accretion disk wind

180. Mid- and far-infrared fine-structure line sensitivities to hypothetical variability of the fine-structure constant

181. The ESO Large Programme First Stars

182. Science with a 16m VLT: the case for variability of fundamental constan ts

183. Bounds on the fine structure constant variability from FeII absorption lines in QSO spectra

184. The CODEX-ESPRESSO experiment: cosmic dynamics, fundamental physics, planets and much more..

185. UVES radial velocity accuracy from asteroid observations. Implications for the fine structure constant variability

186. First Stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876--032

187. A new approach for testing variations of fundamental constants over cosmic epochs using FIR fine-structure lines

188. First Stars VIII -- Enrichment of the neutron-capture elements in the early Galaxy

189. Primordial Light Element Abundances

190. The isotopic 6Li/7Li ratio in Cen X-4 and the origin of Li in X-ray binaries

191. Variations in the lithium abundances of turn off stars in the globular cluster 47 Tuc

192. A new measure of Delta alpha/alpha at redshift z = 1.84 from very high resolution spectra of Q1101-264

193. High-Precision Measurements of Delta alpha/alpha from QSO Absorption Spectra

194. First stars VII. Lithium in extremely metal poor dwarfs

195. First stars X. The nature of three unevolved Carbon-Enhanced Metal-Poor stars

196. First stars IX -Mixing in extremely metal-poor giants. Variation of the 12C/13C, [Na/Mg] and [Al/Mg] ratios

197. VLT/UVES constraints on the carbon isotope ratio 12C/13C at z=1.15 toward the quasar HE 0515-4414

198. Exploring variations in the fundamental constants with ELTs: The CODEX spectrograph on OWL

199. Most precise single redshift bound to the variability of the fine-structure constant

200. Most precise single redshift bound to Delta alpha/alpha

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