Tracing the Galactic spiral structure with embedded clusters
Denilso Camargo, Charles Bonatto, Eduardo Bica

TL;DR
This study uses embedded clusters to map the Milky Way's spiral arms, supporting a four-arm model and providing detailed distances and locations of clusters within these structures.
Contribution
It reports the discovery of 7 new embedded clusters and demonstrates their effectiveness in tracing the Galaxy's spiral arms, refining the understanding of Galactic structure.
Findings
Supports a four-armed spiral pattern in the Milky Way.
Locates clusters predominantly in the Perseus and Outer arms.
Provides distance estimates for key spiral arm segments.
Abstract
In the present work we investigate the properties of 18 embedded clusters (ECs). The sample includes 11 previously known clusters and we report the discovery of 7 ECs on WISE images, thus complementing our recent list of 437 new clusters. The main goal is to use such clusters to shed new light on the Galactic structure by tracing the spiral arms with cluster distances. Our results favour a four-armed spiral pattern tracing three arms, Sagitarius-Carina, Perseus, and the Outer arm. The Sagitarius-Carina spiral arm is probed in the borderline of the third and fourth quadrants at a distance from the Galactic centre of kpc adopting kpc, or kpc for kpc. Most ECs in our sample are located in the Perseus arm that is traced in the second and third quadrants and appear to be at Galactocentric distances in the range kpc or…
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