Issue |
A&A
Volume 508, Number 3, December IV 2009
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---|---|---|
Page(s) | 1313 - 1330 | |
Section | Galactic structure, stellar clusters, and populations | |
DOI | https://doi.org/10.1051/0004-6361/200913327 | |
Published online | 04 November 2009 |
Online Material
Figure 21: The flare event observed on Star #11 (2MASS J05352550-0545448 = NR Ori) on December 10th, 2006 at 3:30 UT in the I band (upper panel). The simultaneous J light curve (bottom panel) does not show any clear variation. |
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Open with DEXTER |
Figure 22: Light curves in the R, I, and J band of the five variable stars for which we could not find any reliable period. |
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Open with DEXTER |
Figure 23: Hectochelle spectra in the H region of our targets (black lines) with the best templates superimposed (thin red lines). The H emission has been cut in order to display the photospheric absorption lines. The Id number is marked in the top-left corner of each box. |
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Open with DEXTER |
Figure 24: Hectochelle spectra in the Mg I b region of our targets (black lines) with the best templates superimposed (thin red lines). The Id number is marked in the top-left corner of each box. |
|
Open with DEXTER |
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