A New Feature of the Galaxy Revealed by 3D Dust Mapping

Autor(en)

A. A. Goodman, J. Alves, C. Zucker, J. S. Speagle, S. Meingast, T. Robitaille, D. P. Finkbeiner, E. P. Schlafly, G. M. Green

Abstrakt

We present a new, very large, highly-elongated, undulating, gaseous

structure lying just beyond the current orbit of the Sun in the Milky

Way. The structure was discovered using 3D-dust mapping techniques, and

it encompasses several star-forming regions formerly associated with

"Gould's Belt" and the "Local Arm" of the Galaxy. Gaia data, along with

several other large surveys, were critical to this discovery. We will

present several three-dimensional views for this new object, and

speculate on its origins.

Organisation(en)

Institut für Astrophysik

Externe Organisation(en)

Harvard University, Aperio Software, Lawrence Berkeley National Laboratory, Stanford University

Journal

Bulletin of the American Astronomical Society

Band

52

ISSN

0002-7537

Publikationsdatum

01-2020

Peer-reviewed

Ja

ÖFOS 2012

103003 Astronomie, 103004 Astrophysik

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