VLT/NACO adaptive optics imaging of the Herbig Ae star HD 100453
Astronomy and Astrophysics, ISSN: 0004-6361, Vol: 445, Issue: 1, Page: 331-335
2006
- 28Citations
- 8Captures
- 1Mentions
Metric Options: Counts1 Year3 YearSelecting the 1-year or 3-year option will change the metrics count to percentiles, illustrating how an article or review compares to other articles or reviews within the selected time period in the same journal. Selecting the 1-year option compares the metrics against other articles/reviews that were also published in the same calendar year. Selecting the 3-year option compares the metrics against other articles/reviews that were also published in the same calendar year plus the two years prior.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Article Description
We report the detection of a companion candidate to the Herbig Ae star HD 100453, using the NACO instrument at the VLT UT4. The separation between the companion candidate and HD 100453 is 1.′06, and their brightness contrast is 5.1 mag at K and 4.2 mag at Bry. We discuss the possible nature of the newly detected star based on near-infrared photometry. The photometric data are consistent with a 0.3 M companion to HD 100453, corresponding to a spectral type of M3-M5. This detection could have important implications for the structure of the disk around HD 100453. © ESO 2005.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=29444438455&origin=inward; http://dx.doi.org/10.1051/0004-6361:20054122; http://www.aanda.org/10.1051/0004-6361:20054122; http://www.aanda.org/10.1051/0004-6361:20054122/pdf; http://dx.doi.org/10.1051/0004-6361%3A20054122; https://dx.doi.org/10.1051/0004-6361%3A20054122; https://www.aanda.org/articles/aa/abs/2006/01/aa4122-05/aa4122-05.html
EDP Sciences
Provide Feedback
Have ideas for a new metric? Would you like to see something else here?Let us know