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Astron. Astrophys. 359, 601-614 (2000)
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The tip of the red giant branch and distance of the Magellanic Clouds: results from the DENIS survey
M.-R.L. Cioni 1,
R.P. van der Marel 2,
C. Loup 3 and
H.J. Habing 1
1 Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, The Netherlands
2 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
3 Institute d'Astrophysique de Paris, CNRS, 98 bis Bd. Arago, 75014 Paris, France
Received 16 March 2000 / Accepted 4 May 2000
Abstract
We present a precise determination of the apparent magnitude of the
tip of the red giant branch (TRGB) in the I
( m), J
( m), and
( m)
bands from the luminosity function of a sample of data extracted from
the DENIS catalogue towards the Magellanic Clouds (Cioni et al.
2000a). From the J and
magnitudes we derive bolometric magnitudes
. We present a new algorithm for the
determination of the TRGB magnitude, which we describe in detail and
test extensively using Monte-Carlo simulations. We note that any
method that searches for a peak in the first derivative (used by most
authors) or the second derivative (used by us) of the observed
luminosity function does not yield an unbiased estimate for the actual
magnitude of the TRGB discontinuity. We stress the importance of
correcting for this bias, which is not generally done. We combine the
results of our algorithm with theoretical predictions to derive the
distance modulus of the Magellanic Clouds. We obtain
(formal)
(systematic) for the Large Magellanic
Cloud (LMC), and (formal)
(systematic) for the Small Magellanic
Cloud (SMC). These are among the most accurate determinations of these
quantities currently available, which is a direct consequence of the
large size of our sample and the insensitivity of near infrared
observations to dust extinction.
Key words: methods:
statistical
stars:
evolution
galaxies: Magellanic
Clouds
galaxies: distances and redshifts
Send offprint requests to: mrcioni@strw.leidenuniv.nl
© European Southern Observatory (ESO) 2000
Online publication: July 7, 2000
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