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The Strömgren photometric system, abbreviated also as ''uvbyβ'' or simply ''uvby'', and sometimes referred as Strömgren - Crawford
photometric system In astronomy, a photometric system is a set of well-defined passbands (or optical filters), with a known sensitivity to incident radiation. The sensitivity usually depends on the optical system, detectors and filters used. For each photometric s ...
, is a four-colour medium-
passband A passband is the range of frequency, frequencies or wavelengths that can pass through a Filter (signal processing), filter. For example, a radio receiver contains a bandpass filter to select the frequency of the desired radio signal out of all t ...
photometric system In astronomy, a photometric system is a set of well-defined passbands (or optical filters), with a known sensitivity to incident radiation. The sensitivity usually depends on the optical system, detectors and filters used. For each photometric s ...
plus Hβ (H-beta) filters for determining magnitudes and obtaining
spectral classification ''Spectral'' is a 2016 Hungarian-American military science fiction action film co-written and directed by Nic Mathieu. Written with Ian Fried & George Nolfi, the film stars James Badge Dale as DARPA research scientist Mark Clyne, with Max M ...
of stars. Its use was pioneered by the Danish astronomer Bengt Strömgren in 1956 and was extended by his colleague the American astronomer David L. Crawford in 1958. It is often considered to be a powerful tool and successful investigating the brightness and effective temperature of stars. This photometric system also has a general advantage as it can be used to measure the effects of reddening and interstellar extinction. This system also allows calculation of parameters from the b and y filters (b-y) without the effects of reddening, termed m_1 and c_1.


Wavelength and half-width response functions

The following table shows the characteristics of each of the filters used (represented colors are only approximate): : Note: colors are only approximate and based on wavelength to sRGB representation (when possible).


Indices

There are four main highly applied and technical indices: (b-y); m_1; c_1; and \beta. * m_1 = (v-b) - (b-y) * c_1=(u-v) - (v-b) * \beta = \beta_ - \beta_ Where; * y magnitudes are well-correlated with Johnson-Morgan V magnitudes (its V band). * (b-y) is sensitive to stellar
temperature Temperature is a physical quantity that quantitatively expresses the attribute of hotness or coldness. Temperature is measurement, measured with a thermometer. It reflects the average kinetic energy of the vibrating and colliding atoms making ...
(measure of Paschen continuum). * c_1 is sensitive to the surface gravity (measures Balmer discontinuity strength). * m_1 is sensitive to the
metallicity In astronomy, metallicity is the Abundance of the chemical elements, abundance of Chemical element, elements present in an object that are heavier than hydrogen and helium. Most of the normal currently detectable (i.e. non-Dark matter, dark) matt ...
(measure of line blanketing).


See also

*
Photometric system In astronomy, a photometric system is a set of well-defined passbands (or optical filters), with a known sensitivity to incident radiation. The sensitivity usually depends on the optical system, detectors and filters used. For each photometric s ...
s *
Stellar classification In astronomy, stellar classification is the classification of stars based on their stellar spectrum, spectral characteristics. Electromagnetic radiation from the star is analyzed by splitting it with a Prism (optics), prism or diffraction gratin ...


References


External links


The Asiago Database on Photometric Systems



Stromgren photometric system tutorial

SAGA: Strömgren survey for Asteroseismology and Galactic Archaeology
{{DEFAULTSORT:Stromgren photometric system Photometric systems