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A multi-wavelength analysis of BL Her stars: Models versus Observations

A multi-wavelength analysis of BL Her stars: Models versus Observations

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2922352700

A multi-wavelength analysis of BL Her stars: Models versus Observations

About this item

Full title

A multi-wavelength analysis of BL Her stars: Models versus Observations

Publisher

Cambridge, UK: Cambridge University Press

Journal title

Proceedings of the International Astronomical Union, 2022-12, Vol.18 (S376), p.105-114

Language

English

Formats

Publication information

Publisher

Cambridge, UK: Cambridge University Press

More information

Scope and Contents

Contents

We present new theoretical period–luminosity (PL) and period–radius (PR) relations at multiple wavelengths (Johnson–Cousins–Glass and Gaia passbands) for a fine grid of BL Herculis models computed using mesa-rsp. The non-linear models were computed for periods typical of BL Her stars, i.e. 1 ≤ P(days) ≤ 4, covering a wide range of input parameters:...

Alternative Titles

Full title

A multi-wavelength analysis of BL Her stars: Models versus Observations

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2922352700

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2922352700

Other Identifiers

ISSN

1743-9213

E-ISSN

1743-9221

DOI

10.1017/S1743921323002612

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