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Using photometric variability as our main selection criterion , as well as follow - up spectroscopy , we confirmed 168 previously unidentified pre - main sequence stars that are about 0.6 to 0.9 times the mass of the sun ( M. ) ...
Using photometric variability as our main selection criterion , as well as follow - up spectroscopy , we confirmed 168 previously unidentified pre - main sequence stars that are about 0.6 to 0.9 times the mass of the sun ( M. ) ...
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Our survey for low - mass young stars in the ~ 100,000 stars in our survey area has , on Orion is unique in its repeated observation of average , 12 to 15 data points during this large areas of the sky . The survey is being period ...
Our survey for low - mass young stars in the ~ 100,000 stars in our survey area has , on Orion is unique in its repeated observation of average , 12 to 15 data points during this large areas of the sky . The survey is being period ...
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Spatial distribution of previously unidentified TTS ( solid symbols ) compared to Hipparcosselected stars of O ... The position of the belt stars ( large star symbols ) and the limits of the scan ( dotted lines ) are indicated as ...
Spatial distribution of previously unidentified TTS ( solid symbols ) compared to Hipparcosselected stars of O ... The position of the belt stars ( large star symbols ) and the limits of the scan ( dotted lines ) are indicated as ...
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Bibliographic information
| Title | Science, Volume 291 |
| Editor | John Michels (Journalist) |
| Contributor | American Association for the Advancement of Science |
| Publisher | American Association for the Advancement of Science, 2001 |
| Original from | University of Illinois at Urbana-Champaign |
| Digitized | 2 Apr 2018 |
| Export Citation | BiBTeX EndNote RefMan |