Long slit spectroscopy in M31 (Saglia+, 2010)

Details Long slit spectroscopy in M31 (Saglia+, 2010) Long slit spectroscopy in M31 (Saglia+, 2010)

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35099061s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/509/A61. Originally published in: 2010A&A...509A..61S

Physics

Galaxies: Nearby, Radial Velocities, Equivalent Widths

Scientific paper

The stellar and gas kinematics (Table 2), the equivalent widths of the Hβ gas emission line, plus the EW ratios [OIII]/Hβ and [NI]/NI (Table 3), and the Lick absorption line strength indices (Table 4) of the bulge of M31 presented here have been measured from spectra taken with the Hobby-Eberly Telescope and the Low Resolution Spectrograph. We observed at six position angles, with a slit width of 1.5-arcsec, a spectral resolution of sigma=57km/s and covering the spectral range 4787-5857Å, with seeing values between 1.4 and 2.5-arcsec.
(4 data files).

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