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Far 3 kpc Arm
29 Jan 2020 11Department of Physics, Faculty of Science, Hokkaido University, Kita 10 Nishi 8, Kita-Ku, Sapporo, Hokkaido 060-0810, Japan
Nd AAS Meeting Abstracts
Hi Absorption Toward Hii Regions at Small Galactic
Gas Flow Models in the Milky Way Embedded Bars
Curriculum Vitae (Pdf)
Discovery of a Pair of Classical Cepheids in an Invisible Cluster Beyond the Galactic Bulge I
The Observed Spiral Structure of the Milky Way⋆⋆⋆
334—24October2020 Editor:Joãoalves(
[email protected]
) List of Contents
Photometric Distances to Young Stars in the Inner Galactic Disk II
The Environmental Impact of High- and Low-Mass Stars: from Formation to Main Sequence
254 — 13 February 2014 Editor: Bo Reipurth (
[email protected]
) List of Contents
SEDIGISM: Structure, Excitation, and Dynamics of the Inner Galactic Interstellar Medium
Structure, Excitation, and Dynamics of the Inner Galactic Interstellar Medium
WFIRST SDT Final Report
The Start of the Sagittarius Spiral
Arxiv:1810.08819V2
Download Approximately −3◦ ≤ ` ≤ 5◦ and |B|≤ 0.◦50
The Spiral Structure of the Milky Way
Top View
Catalogue of Observed Tangents to the Spiral Arms in the Milky Way Galaxy
A Molecular Spiral Arm in the Far Outer Galaxy
The Observed Spiral Structure of the Milky Way Distances and Found That the Distribution Is Consistent with the 1988)
II. Statistical Analysis and Galactic Distribution of 6668-Mhz Methanol Masers
Trigonometric Parallaxes to Star-Forming Regions Within 4 Kpc Of
CHIMPS2: Survey Description and 12CO Emission in the Galactic Centre
THE AUSTRALIA TELESCOPE COMPACT ARRAY H I SURVEY of the GALACTIC CENTER
Downloaded from ORCA, Cardiff University's Institutional Repository