The distance to the Leo I dwarf spheroidal galaxy from the Red Giant Branch Tip ⋆

نویسندگان

  • M. Bellazzini
  • N. Gennari
  • F. R. Ferraro
  • A. Sollima
چکیده

We present V and I photometry of a 9.4 ′ × 9.4 ′ field centered on the dwarf spheroidal galaxy Leo I. The I magnitude of the tip of the Red Giant Branch is robustly estimated from two different datasets (I T RGB = 17.97 +0.05 −0.03). From this estimate, adopting [M/H] ≃ −1.2 from the comparison of RGB stars with Galactic templates, we obtain a distance modulus (m − M) 0 = 22.02 ± 0.13, corresponding to a distance D = 254 +16 −19 Kpc.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The Red Giant Branch Tip and Bump of the Leo II dwarf spheroidal galaxy

We present V and I photometry of a 9.4 × 9.4 field centered on the dwarf spheroidal galaxy Leo II. The Tip of the Red Giant Branch is identified at I = 17.83± 0.03 and adopting 〈[M/H ]〉 = −1.53±0.2 from the comparison of RGB stars with Galactic templates, we obtain a distance modulus (m − M)0 = 21.84 ± 0.13, corresponding to a distance D = 233 ± 15 Kpc. Two significant bumps have been detected ...

متن کامل

Pulsating red giant and supergiant stars in the Local Group dwarf galaxy Andromeda I

We have conducted an optical long-term monitoring survey of the majority of dwarf galaxies in the Local Group, with the Isaac Newton Telescope (INT), to identify the long period variable (LPV) stars. LPV stars vary on timescales of months to years, and reach the largest amplitudes of their brightness variations at optical wavelengths, due to the changing temperature. They trace stellar populati...

متن کامل

To appear in ApJL The distance to the Fornax dwarf galaxy using red clump stars, and the discrepancy between red clump and tip of the red giant branch distances

The distance to the Fornax dwarf galaxy using red clump stars, and the discrepancy between red clump and tip of the red giant branch distances ABSTRACT I determine a distance to the Fornax dwarf galaxy using stars in the red clump and at the tip of the red giant branch. They are in very good agreement, with µ 0 = 20.66 mag. Comparing the magnitudes of the tip of the red giant branch and of the ...

متن کامل

Tip of the Red Giant Branch Distance for the Sculptor Group Dwarf ESO 540 - 032 ?

We present the first V I CCD photometry for the Sculptor group galaxy ESO 540-032 obtained at the Very Large Telescope UT1+FORS1. The (I, V − I) colour-magnitude diagram indicates that this intermediatetype dwarf galaxy is dominated by old, metal-poor ([Fe/H]≈ −1.7 dex) stars, with a small population of slightly more metal-rich ([Fe/H]≈ −1.3 dex), young (age 150 − 500 Myr) stars. A discontinuit...

متن کامل

ar X iv : a st ro - p h / 98 12 26 6 v 1 1 4 D ec 1 99 8 Stellar populations in the dwarf spheroidal galaxy Leo I

We present a detailed study of the color magnitude diagram (CMD) of the dwarf spheroidal galaxy Leo I, based on archival Hubble Space Telescope data. Our photometric analysis, confirming previous results on the brighter portion of the CMD, allow us to obtain an accurate sampling of the stellar populations also at the faint magnitudes corresponding to the Main Sequence. By adopting a homogeneous...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008