Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2213
Title: Age Sequence in Small Clusters Associated with Bright-Rimmed Clouds
Authors: Ogura, K
Chauhan, N
Pandey, A. K
Bhatt, B. C
Ojha, D
Itoh, Y
Keywords: Galaxy: open clusters and associations;general ISM: globules ISM: HII regions stars;ormation stars: pre-main sequence
Issue Date: Feb-2007
Publisher: Astronomical Society of Japan
Citation: Publications of the Astronomical Society of Japan, Vol. 59, pp. 199 - 204
Abstract: Bright-rimmed clouds (BRCs) found in HII regions are probable sites of triggered star formation due to compression by ionization/shock fronts, and it is hypothesized that star formation proceeds from the exciting star(s) side outward of the HII region (``small-scale sequential star formation''). In order to quantitatively test this hypothesis we undertook $BVI_\mathrm{c}$ photometry of four BRC aggregates. The amounts of interstellar extinction and reddening for each star were estimated by using $JHK_\mathrm{s}$ photometry. We then constructed reddening-corrected $V/V-I_\mathrm{c}$ color-magnitude diagrams, where the age of each star was derived. All of the stars turned out to be a few tenths to a few Myr old. Although the scatters were large and the numbers of the sample stars are small, we found a clear trend that the stars inside or in the immediate vicinity of the bright rim are younger than those outside it in all four aggregates, confirming the hypothesis in question.
Description: Restricted Access
URI: http://hdl.handle.net/2248/2213
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http://arxiv.org/abs/astro-ph/0611845
Appears in Collections:Publications based on data from IAO, Hanle
IIAP Publications

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