
Segue 3 - Wikipedia
Segue 3 is a faint star cluster of the Milky Way galaxy discovered in 2010 in the data obtained by Sloan Digital Sky Survey. [1] It is located in the Pegasus constellation at the distance of about 17 kpc from the Sun and moves away from it with the velocity of 167.1 ± 1.5 km/s. [2]
Segue 3: a captured, disrupted outer halo globular cluster
When 3 distinct Submitters promote the image, it moves on to the next stage of the process: evaluation for Top Pick status. This requirement, in addition to anonymization of images and distribution to only a subset of them, prevents biases and …
Title: Segue 3: An Old, Extremely Low luminosity Star Cluster in …
Jul 15, 2011 · Abstract: We investigate the kinematic and photometric properties of the Segue 3 Milky Way companion using Keck/DEIMOS spectroscopy and Magellan/IMACS g and r-band imaging. Using maximum likelihood methods to analyze the photometry, we study the structure and stellar population of Segue 3.
Extratidal Members of Segue 3 are Rare and Difficult to Confirm
Jun 20, 2023 · We simulate extratidal members of Segue 3, a sparse, faint, and small, ∼2.6 Gyr halo cluster, and investigate their observational detectability.
Segue 3 - Wikiwand
Segue 3 is a faint star cluster of the Milky Way galaxy discovered in 2010 in the data obtained by Sloan Digital Sky Survey. It is located in the Pegasus constellation at the distance of about 17 kpc from the Sun and moves away from it with the velocity of 167.1 ± 1.5 km/s.
A Multiwavelength Study of the Segue 3 Cluster - IOPscience
Jul 14, 2017 · In this paper, we study Segue 3 with Washington (Section 2.2) and SDSS (Section 2.3) filters, both to provide more wavelength coverage and to reduce the observational uncertainties in the age and metallicity.
clusters: individual (Segue 3) Online-only material: color figures 1. INTRODUCTION Segue 3 (hereafter Seg 3) is a recently discovered Milky Way satellite, initially estimated to have an extremely low luminosity (M V ∼−1.2, ∼250L), a half-light radius of ∼3 pc, and a distance of ∼17 kpc (Belokurov et al. 2010). Five other Milky
Segue 3: the youngest globular cluster in the outer halo
Abstract: Deep Galileo (Telescopio Nazionale Galileo) B, V and I images of Segue 3, reaching V ∼ 25, reveal that it is the youngest globular cluster known so far in the Galaxy. A young age of 3.2 Gyr is found, differently from a previous estimate of 12 Gyr.
Failure – Segue 3 Lyrics - Genius
Aug 13, 1996 · Who produced “Segue 3” by Failure? When did Failure release “Segue 3”? Who wrote “Segue 3” by Failure? 1992-1996. Failure. 1. Submission. 2. Macaque. 3. Something. 4. Screen Man. 5.
Segue 3: the youngest globular cluster in the outer halo
Jun 13, 2013 · Deep Galileo (Telescopio Nazionale Galileo) B, V and I images of Segue 3, reaching V ∼ 25, reveal that it is the youngest globular cluster known so far in the Galaxy. A young age of 3.2 Gyr is found, differently from a previous estimate of 12 Gyr.