TY - JOUR
T1 - The DDO IVC distance project
T2 - Survey description and the distance to G139.6+47.6
AU - Burns, Christopher R.
AU - Tycner, Christopher
AU - McClure, Megan
AU - Blindert, Kris
AU - McNaughton, Rosemary
AU - Gladders, Michael D.
AU - Attard, Allen
PY - 2003/5
Y1 - 2003/5
N2 - We present a detailed analysis of the distance determination for one intermediate-velocity cloud (IVC, G139.6+47.6) from the ongoing DDO IVC Distance Project. Stars along the line of sight to G139.6+47.6 are examined for the presence of sodium absorption attributable to the cloud, and the distance bracket is established by astrometric and spectroscopic parallax measurements of demonstrated foreground and background stars. We detail our strategy regarding target selection, observational setup, and analysis of the data, including a discussion of wavelength calibration and sky subtraction uncertainties. We find a distance estimate of 129 ± 10 pc for the lower limit and 257-33+211 for the upper limit, Given the high number of stars showing absorption due to this IVC, we also discuss the small-scale covering factor of the cloud and the likely significance of nondetections for subsequent observations of this and other similar IVCs. Distance measurements of the remaining targets in the DDO IVC project will be detailed in a companion paper.
AB - We present a detailed analysis of the distance determination for one intermediate-velocity cloud (IVC, G139.6+47.6) from the ongoing DDO IVC Distance Project. Stars along the line of sight to G139.6+47.6 are examined for the presence of sodium absorption attributable to the cloud, and the distance bracket is established by astrometric and spectroscopic parallax measurements of demonstrated foreground and background stars. We detail our strategy regarding target selection, observational setup, and analysis of the data, including a discussion of wavelength calibration and sky subtraction uncertainties. We find a distance estimate of 129 ± 10 pc for the lower limit and 257-33+211 for the upper limit, Given the high number of stars showing absorption due to this IVC, we also discuss the small-scale covering factor of the cloud and the likely significance of nondetections for subsequent observations of this and other similar IVCs. Distance measurements of the remaining targets in the DDO IVC project will be detailed in a companion paper.
KW - ISM: clouds
KW - ISM: individual (G139.6+47.6)
KW - ISM: structure
KW - Stars: distances
KW - Techniques: spectroscopic
UR - http://www.scopus.com/inward/record.url?scp=0042762084&partnerID=8YFLogxK
U2 - 10.1086/374365
DO - 10.1086/374365
M3 - Review article
AN - SCOPUS:0042762084
SN - 0004-6256
VL - 125
SP - 2584
EP - 2589
JO - Astronomical Journal
JF - Astronomical Journal
IS - 5 1769
ER -