Three-dimensional analysis of the minispiral at the galactic center: orbital parameters, periods, and the mass of the black hole

In this paper we simultaneously fit the orbits and line-of-sight velocities of the ionized gas around the supermassive black hole, Sagittarius A* (Sgr A*), at the center of the Milky Way. The data we use are taken with the K-band Multi Object Spectrograph (KMOS), presented in Feldmeier-Krause et al....

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Bibliographic Details
Main Authors: Nitschai, Maria Selina (Author) , Neumayer, Nadine (Author) , Feldmeier-Krause, Anja (Author)
Format: Article (Journal)
Language:English
Published: 2020 June 15
In: The astrophysical journal
Year: 2020, Volume: 896, Issue: 1
ISSN:1538-4357
DOI:10.3847/1538-4357/ab8ea8
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.3847/1538-4357/ab8ea8
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Author Notes:Maria Selina Nitschai, Nadine Neumayer, and Anja Feldmeier-Krause
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Summary:In this paper we simultaneously fit the orbits and line-of-sight velocities of the ionized gas around the supermassive black hole, Sagittarius A* (Sgr A*), at the center of the Milky Way. The data we use are taken with the K-band Multi Object Spectrograph (KMOS), presented in Feldmeier-Krause et al., and cover the central ∼2 pc of the Milky Way. From the brightest gas emission line in the K-band, the Brγ line, we derive the spatial distribution and line-of-sight velocities of the gas in the minispiral. Using the flux distribution and the line-of-sight velocity information, we perform a fit to the three main gas streamers in the minispiral, the Northern Arm, Eastern Arm, and Western Arc, using a Bayesian modeling method, and are able to reconstruct the three-dimensional orbits of these gas streamers. With the best-fit orbital parameters and the measured line-of-sight velocities, we constrain the mass of Sgr A*. The orbit of the Eastern Arm is the one that is best constrained using our data.
Item Description:Gesehen am 13.08.2020
Physical Description:Online Resource
ISSN:1538-4357
DOI:10.3847/1538-4357/ab8ea8