Measuring spatially resolved gas-to-dust ratios in AGB stars

S. Srinivasan; F. Kemper; Sofia WallstrÃ¶m; T. Dharmawardena; B. RodrÃ­guez Marquina; P. Scicluna; S. Srinivasan; F. Kemper; Franz Kerschbaum; Martin Groenewegen; Hans Olofsson

Measuring spatially resolved gas-to-dust ratios in AGB stars

S. Srinivasan, F. Kemper, Sofia WallstrÃ¶m, T. Dharmawardena, B. RodrÃguez Marquina, P. Scicluna, S. Srinivasan, F. Kemper, Franz Kerschbaum, Martin Groenewegen, Hans Olofsson

Producción científica: Informe/libro › Libro › revisión exhaustiva

Resumen

Gas-to-dust ratios in Asymptotic Giant Branch (AGB) stars are used to calculate gas masses from measured dust masses and vice versa, but can vary widely and are rarely directly measured. In this work, we present spatially resolved gas and dust masses for a sample of 8 nearby AGB stars, using JCMT CO-line and continuum observations, and compare them. This serves as a pilot study for the Nearby Evolved Stars Survey (NESS; PI: P. Scicluna) project which will provide similar observations of ∼1/4400 AGB stars in a volume-limited sample.

Idioma original	Español
Estado	Publicada - 1 ene. 2019
Publicado de forma externa	Sí

Citar esto

@book{c933b6b780864f9c892a2e98d200fd8d,

title = "Measuring spatially resolved gas-to-dust ratios in AGB stars",

abstract = "Gas-to-dust ratios in Asymptotic Giant Branch (AGB) stars are used to calculate gas masses from measured dust masses and vice versa, but can vary widely and are rarely directly measured. In this work, we present spatially resolved gas and dust masses for a sample of 8 nearby AGB stars, using JCMT CO-line and continuum observations, and compare them. This serves as a pilot study for the Nearby Evolved Stars Survey (NESS; PI: P. Scicluna) project which will provide similar observations of ∼1/4400 AGB stars in a volume-limited sample.",

author = "S. Srinivasan and F. Kemper and Sofia Wallstr{\~A}¶m and T. Dharmawardena and {Rodr{\~A}guez Marquina}, B. and P. Scicluna and S. Srinivasan and F. Kemper and Franz Kerschbaum and Martin Groenewegen and Hans Olofsson",

year = "2019",

month = jan,

day = "1",

language = "Espa{\~n}ol",

}

TY - BOOK

T1 - Measuring spatially resolved gas-to-dust ratios in AGB stars

AU - Srinivasan, S.

AU - Kemper, F.

AU - WallstrÃ¶m, Sofia

AU - Dharmawardena, T.

AU - RodrÃguez Marquina, B.

AU - Scicluna, P.

AU - Srinivasan, S.

AU - Kemper, F.

AU - Kerschbaum, Franz

AU - Groenewegen, Martin

AU - Olofsson, Hans

PY - 2019/1/1

Y1 - 2019/1/1

N2 - Gas-to-dust ratios in Asymptotic Giant Branch (AGB) stars are used to calculate gas masses from measured dust masses and vice versa, but can vary widely and are rarely directly measured. In this work, we present spatially resolved gas and dust masses for a sample of 8 nearby AGB stars, using JCMT CO-line and continuum observations, and compare them. This serves as a pilot study for the Nearby Evolved Stars Survey (NESS; PI: P. Scicluna) project which will provide similar observations of ∼1/4400 AGB stars in a volume-limited sample.

AB - Gas-to-dust ratios in Asymptotic Giant Branch (AGB) stars are used to calculate gas masses from measured dust masses and vice versa, but can vary widely and are rarely directly measured. In this work, we present spatially resolved gas and dust masses for a sample of 8 nearby AGB stars, using JCMT CO-line and continuum observations, and compare them. This serves as a pilot study for the Nearby Evolved Stars Survey (NESS; PI: P. Scicluna) project which will provide similar observations of ∼1/4400 AGB stars in a volume-limited sample.

M3 - Libro

BT - Measuring spatially resolved gas-to-dust ratios in AGB stars

ER -