Other
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..33590347d&link_type=abstract
VizieR On-line Data Catalog: J/A+A/359/347. Originally published in: 2000A&A...359..347D
Other
Clusters: Globular, Clusters: Open, Reddening, Stars: Distances
Scientific paper
Table 2 lists the galactic globular cluster, as follows: (1) name of object, (2) and (3) galactic coordinates, (4) distance from the sun, (5) reddening derived from dust 100μm emission E(B-V)FIR, (6) E(B-V) derived from the light emitted by the cluster members, and (7) ΔE(B-V) which is the difference between E(B-V)FIR and E(B-V). Table 3 lists the galactic old open clusters, as follows: (1) name of object, (2 and (3) galactic coordinates, (4) distance from the sun, (5) age, (6) E(B-V)FIR, (7) E(B-V), and (8) ΔE(B-V). Assuming the Milky Way dust layer height to be |Z'|=200pc, Table 4 presents the 60 clusters with ΔE(B-V)>0.30, showing their height from the Plane |Z'|, the distance in the cluster line of sight from the true Plane up to the dust layer edge dlayer, and the path length behind the cluster up to the disk border dbck. They are separated in two groups, one formed by clusters within the dust layer (10 globular and 33 old open clusters) and the other by clusters outside it (15 globular and 2 old open clusters). (3 data files).
Bica Eduardo
Dutra Carlos M.
No associations
LandOfFree
Reddening in open and globular clusters (Dutra+, 2000) 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 Reddening in open and globular clusters (Dutra+, 2000), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Reddening in open and globular clusters (Dutra+, 2000) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-765295