Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-22T17:41:26.679Z Has data issue: false hasContentIssue false

BAaDE: The Bulge Asymmetries and Dynamical Evolution survey

Published online by Cambridge University Press:  14 May 2020

Loránt O. Sjouwerman
Affiliation:
National Radio Astronomy Observatory, P.O. Box O, Socorro, NM, U.S.A. email: [email protected]
Ylva M. Pihlström
Affiliation:
University of New Mexico, AlbuquerqueNM, USA
Michael C. Stroh
Affiliation:
University of New Mexico, AlbuquerqueNM, USA Northwestern University, EvanstonIL, USA
Megan O. Lewis
Affiliation:
University of New Mexico, AlbuquerqueNM, USA
Mark J Claussen
Affiliation:
National Radio Astronomy Observatory, P.O. Box O, Socorro, NM, U.S.A. email: [email protected]
Adam C. Trapp
Affiliation:
University of California, Los AngelesCA, USA
R. Michael Rich
Affiliation:
University of California, Los AngelesCA, USA
Mark R. Morris
Affiliation:
University of California, Los AngelesCA, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Bulge Asymmetries and Dynamical Evolution (BAaDE) survey aims to use circumstellar SiO maser line-of-sight velocities as probes for the Galactic gravitational potential and dynamical structure. The SiO masers are detected at a high rate in specific color-selected MSX infrared sources. Furthermore, the SiO maser properties and line ratios, in combination with infrared spectral energy distributions and location in the Galaxy, will statistically yield detailed information on population and evolution of low- to intermediate-mass evolved stars in the Galaxy.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Habing, H. J. 1996, A&AR, 7, 97Google Scholar
Habing, H. J., Sevenster, M. N., Messineo, M., van de Ven, G., & Kuijken, K. 2006, A&A 458, 151Google Scholar
Lewis, M. O., et al., in preparationGoogle Scholar
Pihlström, Y. M., Sjouwerman, L. O., Claussen, M. J, Morris, M. R., Rich, R. M., van Langevelde, H. J., & Quiroga-Nuñez, L. H. 2018, ApJ 868, 7210.3847/1538-4357/aae77dCrossRefGoogle Scholar
Sjouwerman, L. O., Capen, C., & Claussen, M. J. 2009, ApJ 705, 155410.1088/0004-637X/705/2/1554CrossRefGoogle Scholar
Sjouwerman, L. O., Pihlström, Y. M., Rich, R. M., Claussen, M. J., & Morris, M. R. 2018, IAU Symposium 336, 180Google Scholar
Sjouwerman, L. O., et al., in preparationGoogle Scholar
Stroh, M. C., Pihlström, Y. M., Sjouwerman, L. O., Claussen, M. J., Morris, M. R., & Rich, R. M. 2018, ApJ 862, 153CrossRefGoogle Scholar
Stroh, M. C., Pihlström, Y. M., Sjouwerman, L. O., Lewis, M. O., Claussen, M. J., Morris, M. R., & Rich, R. M. 2019, ApJ, acceptedGoogle Scholar
Trapp, A. C., Rich, R. M., Morris, M. R., Sjouwerman, L. O., Pihlström, Y. M., Claussen, M. J., & Stroh, M. C. 2018, ApJ 862, 153Google Scholar