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Grant: Discovery Grants Program - Individual

Brandon University

$15,000.00

Modelling the gaseous disk of the milky way galaxy

FY 2007-08

Summary
This is a proposal to train graduate students in radio astronomy. They will participate in a new generation of large-scale radio surveys observed with the world's largest telescopes, and make discoveries of new phenomena in interstellar space. A community with a strong foundation in radio astronomy is necessary for Canada to remain at the forefront of interstellar medium astrophysics, a position we hold with our leadership in ongoing international radio surveys of the sky.This proposal outlines a research program that reinvigorates a field that essentially became dormant three decades ago, and pioneers new inroads into understanding the structure of our home galaxy, the Milky Way. Radio telescopes reveal that atomic hydrogen gas fills the volume of our galactic home. This gas is widespread and an excellent tool for mapping spiral structure and motions in the Galaxy, as it responds with fluid-like consistency to the gravitational field of the MW's population of stars. However, understanding what our Galaxy actually looks like from afar is akin to being asked to map an entire forest when tied to a single tree within its boundaries. To tackle the challenge of visualizing the Milky Way, I propose to quantitatively model radio observations of atomic hydrogen. A mathematical "model" of a galaxy, complete with features known to exist in the Milky Way, is constructed and "observed" in the computer with a simulated radio telescope. These model observations are then compared to real ones, and numerical parameters that make up the model galaxy are varied until the real data are best reproduced. With these "fitted" models, we can trace our Galaxy's rotation, and make new visual maps of our Galaxy's spiral arms, giving us an accurate "big-picture" of the Milky Way's gaseous structure and dynamics.The modelling approach proposed will ultimately give us the best birds-eye view of our Galaxy yet, and will advance our understanding of the cosmic gas that exists between the stars, and the interplay between these two populations.
Program
Discovery Grants Program - Individual
Location
Manitoba, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data

As published

Application id
338831-2007
Name nom
Foster, TylerJohn
Department département
Physics and Astronomy
Organization id
20
Institution établissement
Brandon University
Province en
Manitoba
Province fr
Manitoba
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2007
Competition year année de concours
2007
Award amount
15000
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
17
Committee name en
Space & Astronomy
Committee name fr
Rech. spatiale et astronomie
Area of application code
1204
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Space and astronomy
Area of application fr
Sciences spatiales et astronomie
Research subject code
3203
Research subject group en
Astronomy and astrophysics
Research subject group fr
Astronomie et astrophysique
Research subject en
Galactic
Research subject fr
Galactique
Partie
1
Nb partie
2
Application title
Modelling the gaseous disk of the milky way galaxy
Keyword
NA
Application summary
This is a proposal to train graduate students in radio astronomy. They will participate in a new generation of large-scale radio surveys observed with the world's largest telescopes, and make discoveries of new phenomena in interstellar space. A community with a strong foundation in radio astronomy is necessary for Canada to remain at the forefront of interstellar medium astrophysics, a position we hold with our leadership in ongoing international radio surveys of the sky.This proposal outlines a research program that reinvigorates a field that essentially became dormant three decades ago, and pioneers new inroads into understanding the structure of our home galaxy, the Milky Way. Radio telescopes reveal that atomic hydrogen gas fills the volume of our galactic home. This gas is widespread and an excellent tool for mapping spiral structure and motions in the Galaxy, as it responds with fluid-like consistency to the gravitational field of the MW's population of stars. However, understanding what our Galaxy actually looks like from afar is akin to being asked to map an entire forest when tied to a single tree within its boundaries. To tackle the challenge of visualizing the Milky Way, I propose to quantitatively model radio observations of atomic hydrogen. A mathematical "model" of a galaxy, complete with features known to exist in the Milky Way, is constructed and "observed" in the computer with a simulated radio telescope. These model observations are then compared to real ones, and numerical parameters that make up the model galaxy are varied until the real data are best reproduced. With these "fitted" models, we can trace our Galaxy's rotation, and make new visual maps of our Galaxy's spiral arms, giving us an accurate "big-picture" of the Milky Way's gaseous structure and dynamics.The modelling approach proposed will ultimately give us the best birds-eye view of our Galaxy yet, and will advance our understanding of the cosmic gas that exists between the stars, and the interplay between these two populations.