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A&A 373, 56-62 (2001)
DOI: 10.1051/0004-6361:20010598
The oxygen abundance distribution in M 101
L. S. PilyuginMain Astronomical Observatory of National Academy of Sciences of Ukraine, Goloseevo, 03680 Kiev-127, Ukraine
(Received 15 March 2001 / Accepted 23 April 2001 )
Abstract
The well-observed spiral galaxy M 101 was considered. The radial
distributions
of oxygen abundances determined in three different ways (with the classic
-method, with the R23-method, and with the P-method) were
compared. It was found that the parameters (the central oxygen abundance and the
gradient) of the radial (O/H)P abundance distribution are close to
those of the (O/H)
abundance distribution. The parameters of the
(O/H)R23 abundance distribution differ significantly from those of the
(O/H)
abundance distribution: the central (O/H)R23 oxygen
abundance is higher by around 0.4 dex and the gradient is steeper by a factor
of around 1.5 as compared to those values in the (O/H)
abundance
distribution.
The dispersion in (O/H)P abundance at fixed radius is rather small,
~0.08 dex, and is equal to that in (O/H)
abundance.
The dispersion in (O/H)R23 abundance at fixed radius is appreciably
larger, ~0.16 dex, compared to that in (O/H)
abundance.
It has been shown that the extra dispersion in (O/H)R23 abundances
is an artifact and reflects scatter in excitation parameter P at fixed radius.
Key words: galaxies: abundances -- galaxies: ISM -- galaxies: spiral -- galaxies: individual: M 101
Offprint request: L. S. Pilyugin, pilyugin@mao.kiev.ua
SIMBAD Objects
© ESO 2001
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