Quantitative interpretation of the morphology of NGC 1288

Details Quantitative interpretation of the morphology of NGC 1288 Quantitative interpretation of the morphology of NGC 1288

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...352l..36f&link_type=abstract

Astronomy and Astrophysics, v.352, p.L36-L39 (1999)

Astronomy and Astrophysics

Astrophysics

3

Galaxies: Individual: Ngc 1288, Galaxies: Kinematics And Dynamics, Galaxies: Photometry, Cosmology: Dark Matter

Scientific paper

We present a quantitative photometry of the bulge and disk of NGC 1288.
We deduce from the multiplicity of spiral arms, using arguments of
density wave theory, that NGC 1288 must be imbedded in a dark halo.
Based on observations collected at the European Southern Observatory,
Paranal, Chile (VLT UT1 Commissioning Program).

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