Poster Open Access

# Relation of Observable Stellar Parameters to Mass-Loss Rate of AGB Stars in the LMC

Prager, Henry; Willson, Lee Anne; Marengo, Massimo; Creech-Eakman, Michelle

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<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
<dc:creator>Prager, Henry</dc:creator>
<dc:creator>Willson, Lee Anne</dc:creator>
<dc:creator>Marengo, Massimo</dc:creator>
<dc:creator>Creech-Eakman, Michelle</dc:creator>
<dc:date>2021-02-26</dc:date>
<dc:description>Mass loss in Asymptotic Giant Branch (AGB) stars has historically proven difficult to characterize accurately.
This is due to a multitude of factors such as differing composition--including chemistry, metallicity, and differences in carbon and oxygen ratios--and differences in their ongoing motion--particularly, differing pulsation modes.
In mass-loss formulations, the mass-loss rate depends on some combinations of stellar parameters, including but not limited to pulsation period, mass, and luminosity.

Using a combination of stellar models and archival data, we have been working at improving the relation between these parameters and the mass-loss rate of the stars. We have used the models and data to improve on the period-mass-luminosity and radius-mass-luminosity relations for M and C stars in both the fundamental and overtone pulsation modes. Current work is focused on accounting for any remaining sources of scatter in the relation between $\dot{M}$ and our parameters $P$, $L$, and $M$.</dc:description>
<dc:identifier>https://zenodo.org/record/4567529</dc:identifier>
<dc:identifier>10.5281/zenodo.4567529</dc:identifier>
<dc:identifier>oai:zenodo.org:4567529</dc:identifier>
<dc:language>eng</dc:language>
<dc:relation>doi:10.5281/zenodo.4567528</dc:relation>
<dc:relation>url:https://zenodo.org/communities/coolstars20half</dc:relation>
<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
<dc:subject>Post main sequence cool stars</dc:subject>
<dc:subject>stars</dc:subject>
<dc:subject>AGB</dc:subject>
<dc:subject>mass loss</dc:subject>
<dc:title>Relation of Observable Stellar Parameters to Mass-Loss Rate of AGB Stars in the LMC</dc:title>
<dc:type>info:eu-repo/semantics/conferencePoster</dc:type>
<dc:type>poster</dc:type>
</oai_dc:dc>

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