The local spiral structure of the Milky Way

Author:

Xu Ye1,Reid Mark2,Dame Thomas2,Menten Karl3ORCID,Sakai Nobuyuki4,Li Jingjing13,Brunthaler Andreas3ORCID,Moscadelli Luca5,Zhang Bo6,Zheng Xingwu7

Affiliation:

1. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China.

2. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA.

3. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany.

4. Mizusawa VLBI (Very Long Baseline Interferometry) Observatory, National Astronomical Observatory of Japan, Japan.

5. INAF (Istituto Nazionale di Astrofisica)–Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy.

6. Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China.

7. Nanjing University, Nanjing 210093, China.

Abstract

Researchers have only recently begun to trace the spiral structure of our Galaxy, the Milky Way, and already find surprising results.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference39 articles.

1. On the origin of the forms and the present condition of some of the clusters of stars, and several of the nebulae;Alexander S.;Astron. J.,1852

2. Some features of Galactic structure in the neighborhood of the Sun;Morgan W. W.;Astron. J.,1952

3. Studies in galactic structure. I. A preliminary determination of the space distribution of the blue giants;Morgan W. W.;Astrophys. J.,1953

4. T. Y. Steiman-Cameron Twin masks of spiral structure? A local perspective in Galaxies and their Masks D. L. Block K. C. Freeman I. Puerari Eds. (Springer New York 2010).

5. H. S. Liszt Determination of Galactic spiral structure at radiofrequencies in The Milky Way Galaxy: Proceedings of the 106th Symposium of the International Astronomical Union Groningen The Netherlands 30 May to 3 June 1983.

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