The distance to G59.7+0.1

Details The distance to G59.7+0.1 The distance to G59.7+0.1

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..242..374x&link_type=abstract

Astrophysical Masers and their Environments, Proceedings of the International Astronomical Union, IAU Symposium, Volume 242, p.

Astronomy and Astrophysics

Astrophysics

1

Ism: Molecules, Galaxy: Kinematics And Dynamics, Galaxy: Structure

Scientific paper

We have measured the distance to the high-mass star-forming region
G59.7+0.1, which harbors the far-infra-red source IRAS 19410+2336. The
distance is 2.20 ± 0.11 kpc and was determined by triangulation
using Very Long Baseline Array (VLBA) observations of 12.2 GHz methanol
masers phase-referenced to two compact extragalactic radio sources.

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