Quick search Find article
Quick search
Find article

The Araucaria Project: A Wide-Field Photometric Survey for Cepheid Variables in NGC 3109*

FREE

Grzegorz Pietrzyński1,2, Wolfgang Gieren1, Andrzej Udalski2, Igor Soszyński1,2, Fabio Bresolin3, Rolf-Peter Kudritzki3, Ronald Mennickent1, Marcin Kubiak2, Michał Szymański2 and Sebastian Hidalgo4

Show affiliations


We have obtained mosaic images of NGC 3109 in the V and I bands on 74 nights, spanning approximately 1 yr. From these data, we have conducted an extensive search for Cepheid variables over the entire field of the galaxy, resulting in the discovery of 113 variables with periods ranging from 3.4 to 31.4 days. In this sample, 76 Cepheids, including many long-period variables, were not known before. For the previously known 45 Cepheids in this galaxy, our data proved that reported periods were wrong for 14 objects; for nearly all other previously known Cepheid variables, we were able to significantly improve on the periods. We construct period-luminosity relations from our data and obtain reddening-corrected distance moduli of 25.72 ± 0.03 mag in V and 25.66 ± 0.03 mag in I. The distance modulus derived from the reddening-independent V-I Wesenheit index turns out to be significantly shorter (25.54 ± 0.03 mag), which indicates that in addition to the foreground extinction of E(B-V) = 0.05 mag, there is an intrinsic to NGC 3109 reddening of about 0.05 mag. Our distance obtained based on the reddening-free Wesenheit magnitudes is consistent with earlier distance determinations of NGC 3109 from Cepheids and the tip of the red giant branch. We improve on our distance and extinction determination combining our optical data with the follow-up near-infrared observations of a subsample of NGC 3109 Cepheids.


Footnote
*  Based on observations obtained with the 1.3 m Warsaw telescope at Las Campanas Observatory.
Subject headings

Cepheids; distance scale; galaxies: distances and redshifts; galaxies: individual (NGC 3109)


Dates

Issue 1 (2006 September 1)

Received 2006 February 27, accepted for publication 2006 May 9



Users also read

What's this?
This innovative new feature generates a list of articles 'also read' by other users based on them reading the original article. Article abstracts citations and references are all considered and weighted accordingly. We hope that this will help you find relevant papers for your research.

  1. The Disc-Halo Structure of NGC 3109
  2. The Araucaria Project: Distance to the Local Group Galaxy NGC 3109 from Near-Infrared Photometry of Cepheids
  3. The Araucaria Project: The Distance to the Local Group Galaxy IC 1613 from Near-Infrared Photometry of Cepheid Variables

View by subject




Export








Please login to access our web services, or create an account if you don't yet have one.

You must have cookies enabled in your web browser to be able to login.

Username
Password

Forgotten your password? Get a new one here.