How far actually is the Galactic Center IRS 13E3 from Sagittarius A${}^{\ast }$?

Abstract

The Galactic Center IRS 13E cluster is a very intriguing IR object located at $\sim 0.13$ pc from Sagittarius A${}^{\ast }$ (Sgr A${}^{\ast }$) in projection distance. There are both arguments for and against the hypothesis that a dark mass like an intermediate mass black hole (IMBH) exists in the cluster. Recently we have detected the rotating ionized gas ring around IRS 13E3, which belongs to the cluster, in the H30$\alpha$ recombination line using ALMA. The enclosed mass is derived to be $M_{encl.}\simeq 2\times 10^4$ $M_{\odot }$, which agrees with an IMBH and is barely less than the astrometric upper limit mass of the IMBH around Sgr A${}^{\ast }$. Because the limit mass depends on the true three-deminsional (3D) distance from Sgr A${}^{\ast }$, it is very important to determine it observationally. However, the 3D distance is indefinite because it is hard to determine the line-of-sight (LOS) distance by usual methods. We would attempt to estimate the LOS distance by spectroscopic informations. The CH${}_3$OH molecule is easily destroyed by cosmic ray around Sgr A${}^{\ast }$. However, we detected a highly excited CH${}_3$OH emission line in the ionized gas stream associated with IRS 13E3. This indicates that IRS 13E3 is located at $r\gtrsim 0.4$ pc from Sgr A${}^{\ast }$.

9 pages, 2 figures, 1 table, Accepted for publication in PASJ

References in corpus (6)

• An Improved Distance and Mass Estimate for Sgr A* from a Multistar Orbit Analysis
• Dynamics of Ionized Gas at the Galactic Center: VLA Observations of the 3D Velocity Field and Location of the Ionized Streams in Sagittarius A West
• The Second Galactic Center Black Hole?; A Possible Detection of Ionized Gas Orbiting around an IMBH embedded in the Galactic Center IRS13E complex
• ALMA Detection of Bipolar Outflows: Evidence for Low Mass Star Formation within 1pc of Sgr A*
• Rotating Ionized Gas Ring around the Galactic Center IRS13E3
• The Nuclear Filaments inside the Circumnuclear Disk in the Central 0.5 pc of the Galactic center

Cited by in corpus (6)

• Resonant Dynamical Friction Around a Super-Massive Black Hole: Analytical Description
• X3: a high-mass Young Stellar Object close to the supermassive black hole Sgr~A*
• The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. II. Kinematic structure
• Trigonometric parallax and proper motion of Sagittarius A* measured by VERA using the new broad-band back-end system OCTAVE-DAS
• Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
• Dynamics of star associations in an SMBH-IMBH system: The case of IRS13 in the Galactic centre