Physics
Scientific paper
Jan 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..73901437c&link_type=abstract
VizieR On-line Data Catalog: J/MNRAS/390/1437. Originally published in: 2008MNRAS.390.1437C
Physics
Abundances: [Fe/H], Radial Velocities, Photometry: Vri, Galaxies: Nearby, Spectroscopy, Stars: Normal
Scientific paper
The spectroscopic fields cover the four stellar streams presented in the Ibata et al. (2007ApJ...671.1591I) M31 extended halo analysis, called Stream "D", "C", "B" and "A", respectively. Multi-object spectroscopic observations with the Keck II telescope and the DEIMOS were obtained in photometric conditions with ~0.8" seeing in 2004 and 2005 September. On 2007 October 8, additional DEIMOS masks were obtained further along the Stream "C" and Stream "D" under ~1" seeing, and cloudy conditions (see Fields F36 and F37 in table 1).
(2 data files).
Chapman Sandra C.
Collins Marieke
Ferguson Andrew
Huxor Avon
Ibata Rodrigo
No associations
LandOfFree
Stellar streams in Andromeda (M31) (Chapman+, 2008) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Stellar streams in Andromeda (M31) (Chapman+, 2008), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar streams in Andromeda (M31) (Chapman+, 2008) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1549529