Hα surface photometry of galaxies in the Virgo cluster III. Observations with INT and NOT 2.5 m telescopes

Details Hα surface photometry of galaxies in the Virgo cluster III. Observations with INT and NOT 2.5 m telescopes Hα surface photometry of galaxies in the Virgo cluster III. Observations with INT and NOT 2.5 m telescopes

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...386..134b&link_type=abstract

Astronomy and Astrophysics, v.386, p.134-139 (2002)

Astronomy and Astrophysics

Astrophysics

25

Galaxies: Photometry, Galaxies: Fundamental Parameters

Scientific paper

We present Hα line imaging observations of 30 galaxies obtained at the 2.5 m INT and NOT telescopes. The observed galaxies are mostly BCD Virgo cluster galaxies. Hα +[NII] fluxes and equivalent widths, as well as images of all the detected targets are presented. With these observations, Hα data are available for =~ 50% of the BCD galaxies listed in the VCC. Based on observations taken at the INT and NOT telescopes, operated on the island of La Palma by the ING and NOT teams in the Spanish Observatorio del Roque de Los Muchachos of the Instituto de Astrofísica de Canarias. Figure 1 is only available in electronic form at http://www.edpsciences.org

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