Presenter Information

Gavin RoseFollow

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University

Shawnee State University

Major

Chemistry

Student Type

Undergraduate Student

Presentation Types

Oral Presentation

Keywords:

Spectroscopy, Black Holes, Galaxies

Abstract

Most galaxies have a massive black hole at their center, and these black holes grow through accreting gas from the galaxy. So we can expect there to be a relation between galaxy mass and black hole mass. Using the spectra of several galaxies, we have measured the masses of their black holes. The gas orbiting the black holes moves at speeds related to the black hole mass, and we can measure the speeds spectroscopically from their Doppler shift. In addition to this, we have observations of the galaxy as a whole with Integral Field Spectroscopy, in which every pixel in the image has a spectrum. This way, we can measure the Doppler shift of each part of the galaxy as it orbits the center, allowing us to measure the mass of the galaxy.

Human Subjects

no

Faculty Mentor Name

Dr. Tim Hamilton

Faculty Mentor Title

Professor

Faculty Mentor Academic Department

Natural Sciences

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The Analysis of Black Hole Masses Through Spectroscopy

Most galaxies have a massive black hole at their center, and these black holes grow through accreting gas from the galaxy. So we can expect there to be a relation between galaxy mass and black hole mass. Using the spectra of several galaxies, we have measured the masses of their black holes. The gas orbiting the black holes moves at speeds related to the black hole mass, and we can measure the speeds spectroscopically from their Doppler shift. In addition to this, we have observations of the galaxy as a whole with Integral Field Spectroscopy, in which every pixel in the image has a spectrum. This way, we can measure the Doppler shift of each part of the galaxy as it orbits the center, allowing us to measure the mass of the galaxy.