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Multi-Facility Study of the Algol-Type Binary d Librae.

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Title: Multi-Facility Study of the Algol-Type Binary d Librae.
Authors: Budding, E.1,2 ebudding@comu.edu.tr, Bakis, V.1, Erdem, A.1, Demircan, O.1, Iliev, L.3, Iliev, I.3, Slee, O. B.4
Source: Astrophysics & Space Science. Apr2005, Vol. 296 Issue 1-4, p371-389. 19p.
Subjects: ALGOL (Computer program language), Light, Astrophysics, Optical resolution, Radio (Medium), Programming languages
Abstract: Various branches of observational information, and related physical problems concerning the bright, relatively close, Algol binary d Lib are discussed. Times of minimum light confirm the classical Algol status, which, combined with the optical and IR photometry of Lazaro et al. (2002), provide the basis for a good understanding of the system’s basic parameters. New spectroscopy from the Coudé spectrograph of the Rozhen Observatory (Bulgaria) allows further information on the model and the mass transfer process. Very high resolution radio observations would also have much to reveal about astrophysics of the semi-detached configuration, not only directly, by informing about the outermost envelopes of the components, but indirectly through high accuracy positional information. We show how this may be related to careful period and astrometric studies. d Lib thus provides a rich source of information on the astrophysics of the Algol configuration. [ABSTRACT FROM AUTHOR]
Copyright of Astrophysics & Space Science is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Multi-Facility Study of the Algol-Type Binary d Librae.
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  Data: <searchLink fieldCode="AR" term="%22Budding%2C+E%2E%22">Budding, E.</searchLink><relatesTo>1,2</relatesTo><i> ebudding@comu.edu.tr</i><br /><searchLink fieldCode="AR" term="%22Bakis%2C+V%2E%22">Bakis, V.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Erdem%2C+A%2E%22">Erdem, A.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Demircan%2C+O%2E%22">Demircan, O.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Iliev%2C+L%2E%22">Iliev, L.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Iliev%2C+I%2E%22">Iliev, I.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Slee%2C+O%2E+B%2E%22">Slee, O. B.</searchLink><relatesTo>4</relatesTo>
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  Data: <searchLink fieldCode="JN" term="%22Astrophysics+%26+Space+Science%22">Astrophysics & Space Science</searchLink>. Apr2005, Vol. 296 Issue 1-4, p371-389. 19p.
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  Data: Various branches of observational information, and related physical problems concerning the bright, relatively close, Algol binary d Lib are discussed. Times of minimum light confirm the classical Algol status, which, combined with the optical and IR photometry of Lazaro et al. (2002), provide the basis for a good understanding of the system’s basic parameters. New spectroscopy from the Coudé spectrograph of the Rozhen Observatory (Bulgaria) allows further information on the model and the mass transfer process. Very high resolution radio observations would also have much to reveal about astrophysics of the semi-detached configuration, not only directly, by informing about the outermost envelopes of the components, but indirectly through high accuracy positional information. We show how this may be related to careful period and astrometric studies. d Lib thus provides a rich source of information on the astrophysics of the Algol configuration. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Astrophysics & Space Science is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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