Published March 6, 2017
| Version v1
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The UBVRI and Infrared Colour Indices of The Sun and Sun-Like Stars
Description
The Sun is not a point source, the photometric observational techniques that are utilised for observing other stars cannot be utilised for the Sun, meaning that it is difficult to derive its colours accurately for astronomical work from direct measurements in different passbands. The solar twins are the best choices because they are the stars that are ideally the same as the Sun in all parameters, and also, their colours are highly similar to those of the Sun. From the 60 articles on the Sun and Sun-like stars in the literature from 1964 until today, the solar colour indices in the optic and infrared regions have been estimated.
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Additional details
References
- Paczyński, B., Szczygieł, D. M., Pilecki, B., & Pojmański, G. 2006, MNRAS, 368, 1311
- Pojmanski, G. 1997, AcA, 47, 467
- Tanrıver, M. 2012, 18th Congress of the National Astronomy and Space Sciences, 1, 253
- Tanrıver, M. 2014a, NewA, 28, 79
- Tanrıver, M. 2014b, NewA, 31, 20
- Tanrıver, M. & Özeren 2016, "The Sun Like Star : HT Vir", The 19th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun