CaltechAUTHORS
  A Caltech Library Service

Stellar and molecular radii of a Mira star: First observations with the Keck Interferometer grism

Eisner, J. A. and Graham, J. R. and Akeson, R. L. and Ligon, E. R. and Colavita, M. M. and Basri, G. and Summers, K. and Ragland, S. and Booth, A. (2007) Stellar and molecular radii of a Mira star: First observations with the Keck Interferometer grism. Astrophysical Journal, 654 (1). L77-L80. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:EISapjl07

[img]
Preview
PDF - Published Version
See Usage Policy.

85Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:EISapjl07

Abstract

Using a new grism at the Keck Interferometer, we obtained spectrally dispersed (R ~ 230) interferometric measurements of the Mira star R Vir. These data show that the measured radius of the emission varies substantially from 2.0 to 2.4 μm. Simple models can reproduce these wavelength-dependent variations using extended molecular layers, which absorb stellar radiation and reemit it at longer wavelengths. Because we observe spectral regions with and without substantial molecular opacity, we determine the stellar photospheric radius, uncontaminated by molecular emission. We infer that most of the molecular opacity arises at approximately twice the radius of the stellar photosphere.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/510717DOIArticle
ORCID:
AuthorORCID
Akeson, R. L.0000-0001-9674-1564
Additional Information:© 2007 The American Astronomical Society. Received 2006 October 9; accepted 2006 November 8; published 2006 December 7. Data presented here were obtained at the W. M. Keck Observatory from telescope time allocated to NASA through the agency’s scientific partnership with Caltech and the University of California. The Observatory was made possible by the generous support of the W. M. Keck Foundation. We thank the entire KI team for making these observations possible and acknowledge the role of MSC software in our data acquisition and analysis. We are indebted to P. Wizinowich, G. Vasisht, and L. Hillenbrand for helping to ensure the successful implementation of the grism, and to P. Hauschildt, J. Carr, and M. Ireland for providing models and molecular opacities used in our analysis.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
W. M. Keck FoundationUNSPECIFIED
Subject Keywords:circumstellar matter; instrumentation: interferometers; stars: AGB and post-AGB; stars: individual (R Virginis); techniques: interferometric; techniques: spectroscopic
Issue or Number:1
Record Number:CaltechAUTHORS:EISapjl07
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:EISapjl07
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:13755
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:09 Jul 2009 22:20
Last Modified:03 Oct 2019 00:44

Repository Staff Only: item control page