Araucaria Project

The Araucaria Project - international science collaboration focused on improving calibration of the extragalactic distance scale based on observations of major distance indicators in several nearby galaxies.

Project 
The Araucaria Project is a collaboration between astronomers from institutions in Europe, Chile and the US. Its principal aim is to provide an improved calibration of the local extragalactic distance scale. In the process of setting up the extragalactic distance scale, the greatest difficulty leading to the currently largest contribution on the systematic uncertainty of the Hubble constant lies in the determination of accurate absolute distances to nearby galaxies. The principal reason for this persisting difficulty is in the unknown dependencies of stellar standard candles, used to measure the distances of nearby galaxies, on the environmental properties of their host galaxies (metallicity, age of the stellar populations etc.). The Araucaria Project is an effort to remedy this situation for several of the most important stellar candles, including Cepheid variables, RR Lyrae stars, red clump giants, and blue supergiants which all have the potential to provide accurate distance determinations to nearby galaxies once their environmental dependencies are well calibrated. Our strategy is to determine precise distances using the various stellar candles to handful of galaxies with widely different environmental parameters, carefully analyze the distance differences between the different stellar candles, and how they vary with the environmental parameters of their host galaxies.

The sample of galaxies include NGC 6822, IC 1613 and NGC 3109 in the Local Group, and NGC 55, NGC 247, NGC 300 and NGC 7793 in the Sculptor Group. All our target galaxies can be resolved into their stellar components with the modern telescopes and instruments available to the project.

Main discoveries 
 The dynamical mass of a classical Cepheid variable star in an eclipsing binary system
 RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system
 An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent, to one per cent

Team members 
 Grzegorz Pietrzyński - PI (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)
 Wolfgang Gieren - PI (Astronomy Departament UdeC, Concepcion, Chile)
 Dariusz Graczyk (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)
 Bogumił Pilecki (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)
Ksenia Suchomska (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)
Gergely Hajdu (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)
 Marek Górski (Astronomy Departament UdeC, Concepcion, Chile)
Paulina Karczmarek (Astronomy Departament UdeC, Concepcion, Chile)
Weronika Narloch (Astronomy Departament UdeC, Concepcion, Chile)
 Rolf Kudritzki (University of Hawaii, United States)
 Fabio Bresolin (University of Hawaii, United States)
 Ian Thompson (Carnegie Institution for Science, United States)
 Jesper Storm (Astrophysikalisches Institut Potsdam, Potsdam, Germany)
 Nicolas Nardetto (Côte d'Azur Observatory, Nice, France)
 Alexandre Gallenne (Astronomy Departament UdeC, Concepcion, Chile)

PhD Students 
 Piotr Wielgórski (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)
 Bartłomiej Zgirski (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)
 Mónica Taormina (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)
Gonzalo Ignacio Rojas García (Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland)

References

External links 
  Araucaria Project Homepage
  Nicolaus Copernicus Astronomical Center Homepage

Category:Astronomy projects