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Title: Trigonometric parallaxes of star forming regions in the Perseus spiral arm

Abstract

We report trigonometric parallaxes and proper motions of water masers for 12 massive star forming regions in the Perseus spiral arm of the Milky Way as part of the Bar and Spiral Structure Legacy (BeSSel) Survey. Combining our results with 14 parallax measurements in the literature, we estimate a pitch angle of 9.°9 ± 1.°5 for a section of the Perseus arm. The three-dimensional Galactic peculiar motions of these sources indicate that on average they are moving toward the Galactic center and slower than the Galactic rotation.

Authors:
; ;  [1];  [2]; ;  [3];  [4]
  1. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany)
  2. Shanghai Astronomical Observatory, Chinese Academy of Science, Shanghai, 200030 (China)
  3. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)
  4. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008 (China)
Publication Date:
OSTI Identifier:
22365529
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 790; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; GALAXIES; INCLINATION; MASERS; MILKY WAY; OPTICS; PROPER MOTION; ROTATION; STARS; THREE-DIMENSIONAL CALCULATIONS; WATER

Citation Formats

Choi, Y. K., Brunthaler, A., Menten, K. M., Hachisuka, K., Reid, M. J., Dame, T. M., and Xu, Y., E-mail: ykchoi@mpifr-bonn.mpg.de, E-mail: ykchoi@kasi.re.kr. Trigonometric parallaxes of star forming regions in the Perseus spiral arm. United States: N. p., 2014. Web. doi:10.1088/0004-637X/790/2/99.
Choi, Y. K., Brunthaler, A., Menten, K. M., Hachisuka, K., Reid, M. J., Dame, T. M., & Xu, Y., E-mail: ykchoi@mpifr-bonn.mpg.de, E-mail: ykchoi@kasi.re.kr. Trigonometric parallaxes of star forming regions in the Perseus spiral arm. United States. doi:10.1088/0004-637X/790/2/99.
Choi, Y. K., Brunthaler, A., Menten, K. M., Hachisuka, K., Reid, M. J., Dame, T. M., and Xu, Y., E-mail: ykchoi@mpifr-bonn.mpg.de, E-mail: ykchoi@kasi.re.kr. Fri . "Trigonometric parallaxes of star forming regions in the Perseus spiral arm". United States. doi:10.1088/0004-637X/790/2/99.
@article{osti_22365529,
title = {Trigonometric parallaxes of star forming regions in the Perseus spiral arm},
author = {Choi, Y. K. and Brunthaler, A. and Menten, K. M. and Hachisuka, K. and Reid, M. J. and Dame, T. M. and Xu, Y., E-mail: ykchoi@mpifr-bonn.mpg.de, E-mail: ykchoi@kasi.re.kr},
abstractNote = {We report trigonometric parallaxes and proper motions of water masers for 12 massive star forming regions in the Perseus spiral arm of the Milky Way as part of the Bar and Spiral Structure Legacy (BeSSel) Survey. Combining our results with 14 parallax measurements in the literature, we estimate a pitch angle of 9.°9 ± 1.°5 for a section of the Perseus arm. The three-dimensional Galactic peculiar motions of these sources indicate that on average they are moving toward the Galactic center and slower than the Galactic rotation.},
doi = {10.1088/0004-637X/790/2/99},
journal = {Astrophysical Journal},
number = 2,
volume = 790,
place = {United States},
year = {Fri Aug 01 00:00:00 EDT 2014},
month = {Fri Aug 01 00:00:00 EDT 2014}
}