Astron. Astrophys. Suppl. Ser.
Volume 125, Number 2, October II 1997
|Page(s)||293 - 301|
|Published online||15 October 1997|
Near infrared H and surface photometry of three Tully-Fisher calibrators: NGC 2366, NGC 2403 and NGC 4236*,**
Università degli Studi di Milano, Via Celoria 16, 20133, Milano, Italy
2 Osservatorio Astronomico di Brera, Via Brera 28, 20121 Milano, Italy
3 MPI für Kernphysik, Postfach 103980, D–69117 Heidelberg, Germany
4 DEMIRM, Observatoire de Paris, 61 Av. de l'Observatoire, 75014 Paris, France
5 present address: Laboratoire d'Astronomie Spatiale, Traverse du Siphon, F-13376 Marseille Cedex 12, France
Send offprint request to: D. Pierini
Accepted: 26 November 1996
Near Infrared H and surface photometry of the three nearby galaxies NGC 2366, NGC 2403 and NGC 4236, used as local calibrators of the Tully-Fisher relation, was obtained using the 2562 NICMOS3 IR array MAGIC attached to the telescope of Calar Alto. The present measurements are compared with the aperture photometry available in the literature. Surface brightness profiles and integrated magnitudes are given.
Key words: galaxies: photometry / galaxies: NGC 2366, NGC 2403, NGC 4236 / infrared: galaxies
based on observations taken at the Calar Alto Observatory, operated by the Max Planck Institut für Astronomie (Heidelberg) jointly with the Spanish National Commission for Astronomy.
The tables are also available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (188.8.131.52) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1997