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Luminous halos surrounding edge-on d...
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Grodnicki, Lauren R.
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Luminous halos surrounding edge-on disk galaxies in the Sloan Digital Sky Survey.
Record Type:
Language materials, printed : Monograph/item
Title/Author:
Luminous halos surrounding edge-on disk galaxies in the Sloan Digital Sky Survey./
Author:
Grodnicki, Lauren R.
Description:
82 p.
Notes:
Source: Dissertation Abstracts International, Volume: 71-07, Section: B, page: 4297.
Contained By:
Dissertation Abstracts International71-07B.
Subject:
Physics, Astrophysics. -
Online resource:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3408531
ISBN:
9781124048680
Luminous halos surrounding edge-on disk galaxies in the Sloan Digital Sky Survey.
Grodnicki, Lauren R.
Luminous halos surrounding edge-on disk galaxies in the Sloan Digital Sky Survey.
- 82 p.
Source: Dissertation Abstracts International, Volume: 71-07, Section: B, page: 4297.
Thesis (Ph.D.)--The University of Chicago, 2010.
We present the first measurement of both major-axis and minor-axis average surface brightness profiles of low-redshift (0.009 ≤ z ≤ 0.1), edge-on Sc-Sd galaxies. The 906 objects in our sample have 90% Petrosian radii between 5 kpc and 15 kpc and were selected from the Fourth Data Release of the Sloan Digital Sky Survey. The minor-axis profile extends to 20 kpc above the disk and a limiting surface brightness of 30 mag/arcsec2 . We demonstrate that this surface brightness profile is best fit by an exponential+power-law with slope 2.3 +/- 0.3 in agreement with simulations and star counts around individual galaxies. We attribute the power-law component to a diffuse stellar halo and present the first measurement of such around isolated, late-type galaxies. We also divide our sample according to physical size and show that the minor-axis power-law slopes of the two size categories do not differ by more than 2sigma, also in agreement with simulations. We find that the average major-axis scale length is reap = 4.37 +/- 0.012 kpc, somewhat larger than the typical value for face-on galaxies (see, for example, Kent (1985)). We also present the first measurement of the ratio of the disk luminosity to that of the halo, and provide a context for this ratio.
ISBN: 9781124048680Subjects--Topical Terms:
1671120
Physics, Astrophysics.
Luminous halos surrounding edge-on disk galaxies in the Sloan Digital Sky Survey.
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Source: Dissertation Abstracts International, Volume: 71-07, Section: B, page: 4297.
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We present the first measurement of both major-axis and minor-axis average surface brightness profiles of low-redshift (0.009 ≤ z ≤ 0.1), edge-on Sc-Sd galaxies. The 906 objects in our sample have 90% Petrosian radii between 5 kpc and 15 kpc and were selected from the Fourth Data Release of the Sloan Digital Sky Survey. The minor-axis profile extends to 20 kpc above the disk and a limiting surface brightness of 30 mag/arcsec2 . We demonstrate that this surface brightness profile is best fit by an exponential+power-law with slope 2.3 +/- 0.3 in agreement with simulations and star counts around individual galaxies. We attribute the power-law component to a diffuse stellar halo and present the first measurement of such around isolated, late-type galaxies. We also divide our sample according to physical size and show that the minor-axis power-law slopes of the two size categories do not differ by more than 2sigma, also in agreement with simulations. We find that the average major-axis scale length is reap = 4.37 +/- 0.012 kpc, somewhat larger than the typical value for face-on galaxies (see, for example, Kent (1985)). We also present the first measurement of the ratio of the disk luminosity to that of the halo, and provide a context for this ratio.
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http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3408531
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