Grid photography of the halo of NGC 4565
Michael W. Davis, E. Feigelson, David W. Latham
Abstract
Michael W. Davis, E. Feigelson, David W. Latham
Abstract
The blue surface brightness profile of the edge-on galaxy NGC 4565 has been measured using grid photography, which is designed for the photometry of very faint features that cover more than a few millimeters on a photographic plate. A halo luminosity of 8.2 plus or minus 1.8 x 10 to the 8th solar luminosities (B) was calculated in an annulus from 9 to 17 kpc from the galaxy center, but no halo was detected beyond 23 kpc, with a luminosity upper limit of 9.7 x 10 to the 8th solar luminosities (B) in a 23-67 kpc annulus.
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The blue surface brightness profile of the edge-on galaxy NGC 4565 has been measured using grid photography, which is designed for the photometry of very faint features that cover more than a few millimeters on a photographic plate. A halo luminosity of 8.2 plus or minus 1.8 x 10 to the 8th solar luminosities (B) was calculated in an annulus from 9 to 17 kpc from the galaxy center, but no halo was detected beyond 23 kpc, with a luminosity upper limit of 9.7 x 10 to the 8th solar luminosities (B) in a 23-67 kpc annulus.
Key concepts: Physics, Halo, Astrophysics, Photometry (optics), Galaxy, Spiral galaxy, Surface brightness, Luminosity