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19992026
most citedThe Distribution of the Elements in the Galactic Disk III. A Reconsideration of Cepheids from l = 30 to 250 Degrees

230 citations · 1.5k across the 53 of their papers we have counts for

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Showing 2024Show all

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astro-ph.SR2024

Circumstellar emission of Cepheids across the instability strip: Mid-infrared observations with VLTI/MATISSE

V. Hocdé, A. Matter, N. Nardetto +14

The circumstellar envelopes (CSE) of Cepheids are still not well characterized despite their potential impact on distance determination via both the period-luminosity relation and…

astro-ph.SR2024

Precise physical parameters of three late-type eclipsing binary giant stars in the Large Magellanic Cloud

G. Rojas García, D. Graczyk, G. Pietrzyński +17

Detached eclipsing binaries (DEBs) allow for the possibility of precise characterization of its stellar components. They offer a unique opportunity to derive their physical paramet…

astro-ph.GA2024★ 38 cited

The VISTA Variables in the Vía Láctea eXtended (VVVX) ESO public survey: Completion of the observations and legacy

R. K. Saito, M. Hempel, J. Alonso-García +143

The ESO public survey VISTA Variables in the Vía Láctea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from . Upon its conclusion, the c…

astro-ph.SR2024

Projection factor and radii of Type II Cepheids

Piotr Wielgórski, Grzegorz Pietrzyński, Wolfgang Gieren +14

Type II Cepheids are old pulsating stars that can be used to trace the distribution of an old stellar population and to measure distances to globular clusters and galaxies within s…

astro-ph.SR2024

Period-luminosity and period-luminosity-metallicity relations for Galactic RR Lyrae stars in the Sloan bands

W. Narloch, G. Hajdu, G. Pietrzynski +6

RR Lyrae stars are excellent tracers of the old population II due to their period-luminosity (PL) and period-luminosity-metallicity (PLZ) relations. While these relations have been…

astro-ph.SR2024

Towards early-type eclipsing binaries as extragalactic milestones: III. Physical properties of the O-type eclipsing binary OGLE LMC-ECL-21568 in a quadruple system

Mónica Taormina, R. -P. Kudritzki, B. Pilecki +8

We present the results from a complex study of an eclipsing O-type binary (Aa+Ab) with the orbital period days, that forms part of a higher-order multiple system…

astro-ph.SR2024

The orbital parameters of the del Cep inner binary system determined using 2019 HARPS-N spectroscopic data

N. Nardetto, V. Hocdé, P. Kervella +11

An inner companion has recently been discovered orbiting the prototype of classical Cepheids, delta Cep, whose orbital parameters are still not fully constrained. We collected new…