Search Publications
What can you Gain From Deconvolution? Observing Faint Galaxies With the Hubble Space Telescope Wide Field Camera
Elson, Rebecca A. W.; Schade, David J.
We describe experiments with deconvolutions of simulations of deep HST Wide Field Camera images containing faint, compact galaxies to determine under what circumstances there is a quantitative advantage to image deconvolution, and explore whether it is (1) helpful for distinguishing between stars and compact galaxies, or between spiral and ellipti…
Internal Ultraviolet Explorer Observations of the white Dwarf Nucleus of the Very Old, Diffuse Planetary Nebula, IW-2
Bruhweiler, F. C.; Feibelman, Walter A.
UV low-dispersion spectra of the central star of the faint planetary nebula, IW-2, were obtained with the IUE. The apparent large diameter of the very diffuse nebula, about half that of the moon, as seen on the Palomar Sky Survey plates by Ishida and Weinberger (1987), indicates this object to be potentially quite evolved, and nearby. The IUE spec…
Silicon Abundances in Population I Giants
Bohm-Vitense, Erika
Silion to carbon abundance ratios for Population I giants were determined from emission lines originating in the transition layers between stellar chromospheres and coronae. For effective temperatures larger than 6200 K we find a group of stars for which the silicon to carbon abundance ratio appears to be increased. These stars are presumably desc…
The Quality of Photometric Information in the HIPPARCOS Input Catalog
Casertano, Stefano; Ratnatunga, Kavan U.; Bell, David J. +1 more
Comparison with independent photoelectric photometry is used to assess the quality of magnitudes and colors in the Hipparcos Input Catalog. These magnitudes and colors will play an important role in the luminosity calibration of Hipparcos stars. We conclude that photoelectric photometry, available for about 37 percent of the catalog, is of uniform…
Planetary Camera Observations of NGC 1275: Discovery of a Central Population of Compact Massive Blue Star Clusters
Holtzman, J. A.; Faber, S. M.; Ewald, S. P. +10 more
We have discovered a population of bright blue pointlike sources within 5 kpc of the nucleus of NGC 1275 using HST Planetary Camera observations. The typical object has M_v_ ~ - 12 to - 14 (H_0_ = 75 km s^-1^ Mpc^-1^ ); the brightest has M_v_ ~ - 16. They are all blue, with V - R <~ 0.3. The color distribution and lack of excess Hα emission are…
NGC 1705. I. Stellar Populations and Mass Loss Via A Galactic Wind
Freeman, K. C.; Meurer, Gerhardt R.; Dopita, Michael A. +1 more
We present a detailed multi-waveband study of the galaxy NGC 1705. The data include optical and ultraviolet spectroscopy, optical and infrared photoelectric aperture photometry, narrowband and broadband images, H I spectra, and data from the IRAS point source catalog. NGC 1705 is shown to be a nearby (D~5 Mpc for H_0_ = 75 km s^-1^ Mpc^-1^) nuclea…
Planetary Camera Observations of the M87 Stellar CUSP
Schneider, Donald P.; Lauer, Tod R.; Faber, S. M. +11 more
Analysis of V and I band HST Planetary Camera images of the giant elliptical galaxy M87 show that its central starlight distribution is consistent with the black hole M_black hole_ = 2.6 X 10^9^ M_sun_ cusp model proposed for M87 by Young et al, [ApJ, 221,721(1978)]. A combined approach of image deconvolution and modeling is used to investigate th…
Planetary Camera Observations of the Central Parsec of M32
Lauer, Tod R.; Faber, S. M.; Currie, Douglas G. +8 more
Analysis of V band HST Planetary Camera images of the elliptical galaxy M32 shows that its nucleus is extremely dense and remains unresolved at even the HST diffraction limit. A combined approach of image deconvolution and model fitting is used to investigate the starlight distribution into limiting radii of 0.04" (0.14 pc at 700 kpc). The logarit…
Hubble Space Telescope Planetary Camera Images of R136
Lauer, Tod R.; Faber, S. M.; Holtzman, Jon A. +9 more
The Planetary Camera of the Hubble Space Telescope has been used to obtain broad and narrowband images of R136, the core of the massive star cluster 30 Doradus in the Large Magellanic Cloud. R136a, the brightest component of R136, is shown to have at least 12 separate components, including the eight originally identified by speckle interferometry.…
Globular Cluster Photometry With the Hubble Space Telescope. I. Description of the Method and Analysis of the Core of 47 TUC
Schneider, Donald P.; Yanny, Brian; Bahcall, John N. +1 more
Accurate photometry for individual post-main-sequence stars in the core of the Galactic globular cluster 47 Tuc is presented and analyzed using an empirical point spread function model and Monte Carlo simulations. A V vs. V-I color-magnitude diagrams is constructed which shows several distinct stellar types, including RGB and HB stars. Twenty-four…