This paper reports the discovery of a helical molecular cloud in the central molecular zone (CMZ) of our Galaxy. This "pigtail" molecular cloud appears at (l, b, V_LSR) ~ (-0.7deg, +0.0deg, -70 to -30 km/s), with a spatial size of ~ (20 pc)^2 and a mass of (2-6) 10^5 solar masses. This is the third helical gaseous nebula found in the Galactic center region to date. Line intensity ratios indicate that the pigtail molecular cloud has slightly higher temperature and/or density than the other normal clouds in the CMZ. We also found a high-velocity wing emission near the footpoint of this cloud. We propose a formation model of the pigtail molecular cloud. It might be associated with a magnetic tube that is twisted and coiled because of the interaction between clouds in the innermost x_1 orbit and ones in the outermost x_2 orbit.
@article{arxiv.1207.4704,
title = {Discovery of the Pigtail Molecular Cloud in the Galactic Center},
author = {Shinji Matsumura and Tomoharu Oka and Kunihiko Tanaka and Makoto Nagai and Kazuhisa Kamegai and Tetsuo Hasegawa},
journal= {arXiv preprint arXiv:1207.4704},
year = {2015}
}
Comments
15 pages, 6 figures, accepted for publication in Astrophysical Journal