We analyze the r-band absolute magnitude and u − r color of low-redshift (z 0.9) to ~0.26 for nearly edge-on galaxies (q < 0.3). When the dimming law ΔM_r ⍺ (log q)^2 is used to create an inclination-corrected sample of bright exponential galaxies, their apparent shapes are consistent with a distribution of mildly noncircular disks, with median short-to-long axis ratio γ approx 0.22 and median disk ellipticity ε approx 0.08
Using photometry and spectroscopy of 183,487 galaxies from the Sloan Digital Sky Survey, we present ...
We characterize the influence that inclination has on the shape and normalization in average dust at...
The emerging light from a galaxy is under the influence of its own interstellar medium, as well as i...
Using the Sloan Digital Sky Survey (SDSS) Data Release 6 (DR6), I study the effects of inclination ...
Using a samples of 61506 spiral galaxies selected from the SDSS DR2, we examine the luminosity funct...
Using a sample of 61,506 spiral galaxies selected from the SDSS DR2, we examine the luminosity funct...
Magnitude-limited samples of spiral galaxies drawn from the Ursa Major and Pisces Clusters are used ...
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral p...
We estimate the distribution of apparent axis ratios $q$ for galaxies in the Sloan Digital Sky Surve...
For a sample of 96,951 galaxies from the Sloan Digital Sky Survey Data Release 3, we study the distr...
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral p...
We investigate the effect of dust on spiral galaxies by measuring the inclination-dependence of opti...
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral p...
The distribution of spiral and bar galaxy inclination angles is expected to be uniform. However, ana...
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral p...
Using photometry and spectroscopy of 183,487 galaxies from the Sloan Digital Sky Survey, we present ...
We characterize the influence that inclination has on the shape and normalization in average dust at...
The emerging light from a galaxy is under the influence of its own interstellar medium, as well as i...
Using the Sloan Digital Sky Survey (SDSS) Data Release 6 (DR6), I study the effects of inclination ...
Using a samples of 61506 spiral galaxies selected from the SDSS DR2, we examine the luminosity funct...
Using a sample of 61,506 spiral galaxies selected from the SDSS DR2, we examine the luminosity funct...
Magnitude-limited samples of spiral galaxies drawn from the Ursa Major and Pisces Clusters are used ...
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral p...
We estimate the distribution of apparent axis ratios $q$ for galaxies in the Sloan Digital Sky Surve...
For a sample of 96,951 galaxies from the Sloan Digital Sky Survey Data Release 3, we study the distr...
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral p...
We investigate the effect of dust on spiral galaxies by measuring the inclination-dependence of opti...
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral p...
The distribution of spiral and bar galaxy inclination angles is expected to be uniform. However, ana...
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral p...
Using photometry and spectroscopy of 183,487 galaxies from the Sloan Digital Sky Survey, we present ...
We characterize the influence that inclination has on the shape and normalization in average dust at...
The emerging light from a galaxy is under the influence of its own interstellar medium, as well as i...