HD 202206: A Circumbinary Brown Dwarf System
Astronomical Journal, ISSN: 0004-6256, Vol: 153, Issue: 6
2017
- 18Citations
- 8Captures
- 5Mentions
Metric Options: CountsSelecting 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
Using Hubble Space Telescope Fine Guidance Sensor astrometry and previously published radial velocity measures, we explore the exoplanetary system HD 202206. Our modeling results in a parallax, milliseconds of arc, a mass for HD 202206 B of, and a mass for HD 202206 c of. HD 202206 is a nearly face-on G + M binary orbited by a brown dwarf. The system architecture that we determine supports past assertions that stability requires a 5:1 mean motion resonance (we find a period ratio,) and coplanarity (we find a mutual inclination,).
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85020744348&origin=inward; http://dx.doi.org/10.3847/1538-3881/aa6d59; https://iopscience.iop.org/article/10.3847/1538-3881/aa6d59; https://dx.doi.org/10.3847/1538-3881/aa6d59; https://validate.perfdrive.com/9730847aceed30627ebd520e46ee70b2/?ssa=e12e922d-de85-4bec-b9f7-b4db9b5fec2d&ssb=22945292239&ssc=https%3A%2F%2Fiopscience.iop.org%2Farticle%2F10.3847%2F1538-3881%2Faa6d59&ssi=05a14141-cnvj-4536-8808-2b8cb7cb9c58&ssk=botmanager_support@radware.com&ssm=6689064944824644828090411283679293&ssn=9657db35c6730089f975eb1516668b4c948da9a60fcd-2cb2-4007-b2ba15&sso=aa8fcdc1-99effaea85e1e70775463d53f368248b4a4b07b96a33a28b&ssp=22273693571736966948173691357580118&ssq=54182526471061604288209927943146696603699&ssr=NTIuMy4yMTcuMjU0&sst=com.plumanalytics&ssu=&ssv=&ssw=&ssx=eyJfX3V6bWYiOiI3ZjYwMDBiN2M0MmExZC00ZTg0LTRjOGYtYmRhYi1lOWM0NzEyM2ZjZjQxNzM2OTA5OTI3Mjc3NTQ3ODI4MTUtYTE2MTk4YjkzNWNjMTdhMjI4MDkiLCJyZCI6ImlvcC5vcmciLCJ1em14IjoiN2Y5MDAwMDhkOWZkYWQtOWYxMS00OGIxLWFhYTctODgzYzQ1NDM1NGUyMS0xNzM2OTA5OTI3Mjc3NTQ3ODI4MTUtNzFmZjJiODMyMjFmZWZmZDI4MDkifQ==
American Astronomical Society
Provide Feedback
Have ideas for a new metric? Would you like to see something else here?Let us know