activity
20092015
most citedOn the fine structure of the Cepheid metallicity gradient in the Galactic thin disk

203 citations · 639 across the 13 of their papers we have counts for

collaborators
Showing 2013Show all

5 papers · 1 filter

astro-ph.GA2013★ 90 cited

Galactic abundance gradients from Cepheids: alpha and heavy elements in the outer disk

B. Lemasle, P. Francois, K. Genovali +11

Context: Galactic abundance gradients set strong constraints to chemo-dynamical evolutionary models of the Milky Way. Given the PL relations that provide accurate distances and the…

astro-ph.SR2013★ 54 cited

On the metallicity distribution of classical Cepheids in the Galactic inner disk

K. Genovali, B. Lemasle, G. Bono +10

We present homogeneous and accurate iron abundances for almost four dozen (47) of Galactic Cepheids using high-spectral resolution (R40,000) high signal-to-noise ratio (S/N $…

astro-ph.SR2013

On the relative distance of Magellanic Clouds using Cepheid NlR and Optical-NIR PW relations

L. Inno, G. Bono, N. Matsunaga +8

We present new estimates of the relative distance of the Magellanic Clouds (MCs) by using NIR and Optical-NIR Cepheid Period Wesenheit (PW) relations. The relative distances are in…

astro-ph.SR2013★ 88 cited

On the distance of the Magellanic Clouds using Cepheid NIR and optical-NIR Period Wesenheit Relations

L. Inno, N. Matsunaga, G. Bono +8

We present the largest near-infrared (NIR) data sets, , ever collected for classical Cepheids in the Magellanic Clouds (MCs). We selected fundamental (FU) and first overtone…

astro-ph.SR2013★ 4 cited

Classical Cepheids, what else?

G. Bono, L. Inno, N. Matsunaga +4

We present new and independent estimates of the distances to the Magellanic Clouds (MCs) using near-infrared (NIR) and optical--NIR period--Wesenheit (PW) relations. The slopes of…