Published on 01 January 2014

XYZUVW predicted positions for J1247-3812 and J1207-3900 vs TWA members.

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Gagné, Jonathan;Faherty, Jackie;Kelle Cruz;Lafrenière, David;Doyon, René;Malo, Lison;Étienne Artigau

Description

These figures show the expected 3-dimensional XYZ and UVW positions of J1207-3900 and J1247-3812 (see Gagné et al. 2014b, first link below; red points; blue lines point to their projections on the 3 planes), compared to the XYZ positions of bona fide members from Malo et al. 2013 (see third link below; green points; their projections are also shown on the 3 planes, and only vertical lines pointing to their XY-or UV-plane projections are shown for clarity). The orange ellipsoid and its projections on the 3 planes represent the 1.5-sigma contour of the spatial model of the moving group in question. The statistical distance predictions from BANYAN II (see Gagné et al. 2014a, second link below) for RVs and distances were used to compute the XYZ or UVW of the two TWA candidates. Measurements of distance and RVs were used in the case of bona fide members. If you use any of these figures, please cite the 3 papers linked below.

Citations (0)

Mentions (0)

Metrics

Dataset Index

0.1

FAIR Score

13%

Citations

0

Mentions

0

Metrics Over Time

Publication Details

DOI

Publisher

figshare

Assigned Domain

Subfield

Astronomy and Astrophysics

Field

Physics and Astronomy

Domain

Physical Sciences

Confidence Score

98%

Source

Open Alex

Keywords

AstrophysicsStellar Astronomy

Normalization Factors

FT

30.77

CTw

1.00

MTw

1.00