ON THE SURVIVAL OF HIGH-ALTITUDE OPEN CLUSTERS WITHIN THE MILKY WAY GALAXY TIDES

• Published in: The Astrophysical journal Vol. 834; no. 1; pp. 58 - 67
• Main Authors: Martinez-Medina, L. A., Pichardo, B., Peimbert, A., Moreno, E.
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01-01-2017; IOP Publishing
• Subjects: Altitude; Astrophysics; Computer simulation; Disruption; Galactic clusters; Galactic disk; Galactic structure; Galaxies; galaxies: kinematics and dynamics; galaxies: spiral; galaxies: structure; Galaxy: disk; High altitude; Life expectancy; Milky Way; Molecular clouds; Open clusters; open clusters and associations: general; Stars & galaxies; Substructures; Survival; Tides
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/834/1/58

ABSTRACT It is a common assumption that high-altitude open clusters live longer compared to clusters moving close to the Galactic plane. This is because, at high altitudes, open clusters are far from the disruptive effects of in-plane substructures, such as spiral arms, molecular clouds, and the bar. However, an important aspect to consider in this scenario is that orbits of high-altitude open clusters will eventually cross the Galactic plane, where the vertical tidal field of the disk is strong. In this work, we simulate the interaction of open clusters with the tidal field of a detailed Milky Way Galactic model at different average altitudes and galactocentric radii. We find that the life expectancy of clusters decreases as the maximum orbital altitude increases and reaches a minimum at altitudes of approximately 600 pc. Clusters near the Galactic plane live longer because they do not experience strong vertical tidal shocks from the Galactic disk; then, for orbital altitudes higher than 600 pc, clusters again start to live longer due to the decrease in the number of encounters with the disk. With our study, we find that the compressive nature of the tides in the arms region and the bar play an important role in the survival of small clusters by protecting them from disruption: clusters inside the arms can live up to twice as long as those outside the arms at similar galactocentric distances.