- #1
bcx
- 2
- 0
Hey,
Been stuck on a problem for over a day now, can't seem to figure it out!
The question reads as follows:
A single high-mass star is surrounded by an HII region that
subtends an angle of 10 arcmin on the sky. The optical colours
of the star suggest it has a bolometric luminosity of 5∙10^(31) W and
it is observed to have a bolometric flux of 4.4∙10(-7) W m-2.
Assuming most of this luminosity is emitted as 10 eV photons, what
is the density of hydrogen gas around the star?
To solve this, I have intially used the formula
to calculate the distance of the high mass star. I have then
calculated the circumference at that distance, and using the
knowledge that the HII subtends an angle of 10 arcminutes, I have
converted the overall circumference into the radius of the HII
region (first by dividing the circumference by (360*6), then
by 2). From this I have determined the volume of the HII region
using 4/3*pi*r^3. Then, I have converted the luminosity of the star
into electron volts (by dividing by 1.6*10^-19), and used the Ionisation formula as follows (the one typically used to find the stromgren radius)
[PLAIN]http://rpmedia.ask.com/ts?u=/math/5/1/2/5128062b3e1ef80caa7cf0ac4f1bb3c2.png
Where I have taken S* as the total luminosity divided by the energy of a single 10eV photon (as stated in the problem).
Then from this I have a value of n^2*beta. where beta is the recombination constant and n is the number desity of hydrogen.
I take an value of beta as 3.1*10^-19 (assuming star is at 8000K), and from this calculated n.
The value is supposed to be 6000/cm^3, but my values always seem to lie in a higher region. I've tried working backwards but all I seem to get is silly values for the temperature of the star. I can't seem to see where I am going wrong. Any light on the situation would be appreciated!
Been stuck on a problem for over a day now, can't seem to figure it out!
The question reads as follows:
A single high-mass star is surrounded by an HII region that
subtends an angle of 10 arcmin on the sky. The optical colours
of the star suggest it has a bolometric luminosity of 5∙10^(31) W and
it is observed to have a bolometric flux of 4.4∙10(-7) W m-2.
Assuming most of this luminosity is emitted as 10 eV photons, what
is the density of hydrogen gas around the star?
To solve this, I have intially used the formula
to calculate the distance of the high mass star. I have then
calculated the circumference at that distance, and using the
knowledge that the HII subtends an angle of 10 arcminutes, I have
converted the overall circumference into the radius of the HII
region (first by dividing the circumference by (360*6), then
by 2). From this I have determined the volume of the HII region
using 4/3*pi*r^3. Then, I have converted the luminosity of the star
into electron volts (by dividing by 1.6*10^-19), and used the Ionisation formula as follows (the one typically used to find the stromgren radius)
[PLAIN]http://rpmedia.ask.com/ts?u=/math/5/1/2/5128062b3e1ef80caa7cf0ac4f1bb3c2.png
Where I have taken S* as the total luminosity divided by the energy of a single 10eV photon (as stated in the problem).
Then from this I have a value of n^2*beta. where beta is the recombination constant and n is the number desity of hydrogen.
I take an value of beta as 3.1*10^-19 (assuming star is at 8000K), and from this calculated n.
The value is supposed to be 6000/cm^3, but my values always seem to lie in a higher region. I've tried working backwards but all I seem to get is silly values for the temperature of the star. I can't seem to see where I am going wrong. Any light on the situation would be appreciated!
Last edited by a moderator: