Spectroscopic Analysis of the IR-Visible Galactic Core

In summary, the massive object at the center of the galaxy, known as Sgr A*, can be seen in both radio waves and X-rays, but not in visible light. However, recent infrared images have been taken of this object. While there have been attempts to do spectroscopy on Sgr A* in the infrared band, it appears that only during flares can enough brightness be observed to successfully analyze its spectral lines.
  • #1
psholtz
136
0
I understand that the massive object at the center of the galaxy is visible in both radio waves and X-rays, although not in visible light.

I also understand that an image has recently been taken of this object in the infrared wavelengths.

Have there been any attempts to do spectroscopy on this object in the IR band?
 
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  • #2
There's lots of different things in the Galactic centre so be a bit more specific.
 
  • #4
qraal said:
There's lots of different things in the Galactic centre so be a bit more specific.
I have in mind Sgr A*, the compact, extremely massive object at the center of the galaxy emitting X-rays and radio waves and which some astronomers believe might be a "black hole"..
 
  • #5
granpa said:
http://Earth'sky.org/space/most-detailed-view-yet-of-milky-way-center

http://www.mpi-hd.mpg.de/hfm/HESS/pages/home/som/2009/12/
Thanks, the second article in particular is informative..

Still, I don't think anyone has done spectroscopy on the IR signals coming from this source, have they?
 
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1. What is spectroscopic analysis?

Spectroscopic analysis is a scientific method used to study the properties and composition of a substance by analyzing its interaction with electromagnetic radiation. In the case of the IR-Visible Galactic Core, spectroscopic analysis can help us understand the chemical makeup and physical processes of this region of the galaxy.

2. Why is the IR-Visible Galactic Core important to study?

The IR-Visible Galactic Core is the central region of our galaxy, where a high concentration of stars, gas, and dust can be found. Understanding the processes and properties of this region can provide valuable insights into the evolution and structure of galaxies in general.

3. How is spectroscopic analysis used to study the IR-Visible Galactic Core?

Spectroscopic analysis involves using instruments called spectrographs to break down the light emitted or absorbed by a substance into its component wavelengths. By studying the specific wavelengths of light that are present in the IR-Visible Galactic Core, scientists can infer the chemical composition, temperature, and motion of the objects in this region.

4. What can we learn from the results of spectroscopic analysis of the IR-Visible Galactic Core?

The results of spectroscopic analysis can provide information about the types of elements present in the IR-Visible Galactic Core, their relative abundances, and their physical conditions. This can help us understand the formation and evolution of stars, gas clouds, and other objects in this region.

5. How does spectroscopic analysis of the IR-Visible Galactic Core contribute to our overall understanding of the universe?

Studying the IR-Visible Galactic Core using spectroscopic analysis can provide valuable data and insights that contribute to our knowledge of the universe. By understanding the chemical and physical processes in this region, we can gain a better understanding of our own galaxy and how it compares to other galaxies in the universe.

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