Observation of the Halo of NGC 3077 Near the "Garland" Region Using the Hubble Space Telescope

Details Observation of the Halo of NGC 3077 Near the "Garland" Region Using the Hubble Space Telescope Observation of the Halo of NGC 3077 Near the "Garland" Region Using the Hubble Space Telescope

2001-03-07

arxiv.org/abs/astro-ph/0103121v1

Astronomy and Astrophysics

Astrophysics

15 pages, 8 figures. Accepted for publication in Astrophysical Journal

Scientific paper

10.1086/321459

We report the detection of upper main sequence stars and red giant branch stars in the halo of an amorphous galaxy, NGC3077. The observations were made using Wide Field Planetary Camera~2 on board the Hubble Space Telescope. The red giant branch luminosity function in I-band shows a sudden discontinuity at I = 24.0 +- 0.1 mag. Identifying this with the tip of the red giant branch (TRGB), and adopting the calibration provided by Lee, Freedman, & Madore (1993) and the foreground extinction of A_B = 0.21 mag, we obtain a distance modulus of (m-M)_0 = 27.93 +- 0.14(random) +- 0.16(sys). This value agrees well with the distance estimates of four other galaxies in the M81 Group. In addition to the RGB stars, we observe a concentration of upper main sequence stars in the halo of NGC3077, which coincides partially with a feature known as the ``Garland''. Using Padua isochrones, these stars are estimated to be <150 Myrs old. Assuming that the nearest encounter between NGC3077 and M81 occurred 280 Myrs ago as predicted by the numerical simulations (Yun 1997), the observed upper main sequence stars are likely the results of the star formation triggered by the M81-NGC3077 tidal interaction.

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