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arXiv · 1710.05441

Maser, infrared and optical emission for late-type stars in the Galactic plane

L. H. Quiroga-Nuñez·H. J. van Langevelde·L. O. Sjouwerman·Y. M. Pihlström·M. J. Reid·A. G. A. Brown·J. A. Green
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Abstract

Radio astrometric campaigns using VLBI have provided distances and proper motions for masers associated with young massive stars (BeSSeL survey). The ongoing BAaDE project plans to obtain astrometric information of SiO maser stars located in the inner Galaxy. These stars are associated with evolved, mass-losing stars. By overlapping optical (Gaia), infrared (2MASS, MSX and WISE) and radio (BAaDE) sources, we expect to obtain important clues on the intrinsic properties and population distribution of late-type stars. Moreover, a comparison of the Galactic parameters obtained with Gaia and VLBI can be done using radio observations on different targets: young massive stars (BeSSeL) and evolved stars (BAaDE).

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L. H. Quiroga-Nuñez, H. J. van Langevelde, L. O. Sjouwerman, Y. M. Pihlström, M. J. Reid, A. G. A. Brown, J. A. Green. 2017-10-16. Maser, infrared and optical emission for late-type stars in the Galactic plane. https://doi.org/10.1017/s1743921317010493

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