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The Hubble Space Telescope Extragalactic Distance Scale Key Project. I. The Discovery of Cepheids and a New Distance to M81
DOI: 10.1086/174172 Bibcode: 1994ApJ...427..628F

Illingworth, Garth D.; Kennicutt, Robert C.; Madore, Barry F. +12 more

We report on the discovery of 30 new Cepheids in the nearby galaxy M81 based on observations using the Hubble Space Telescope (HST). The periods of these Cepheids lie in the range of 10-55 days, based on 18 independent epochs using the HST wide-band F555W filter. The HST F555W and F785LP data have been transformed to the Cousins standard V and I m…

1994 The Astrophysical Journal
eHST 606
HST FOS Spectroscopy of M87: Evidence for a Disk of Ionized Gas around a Massive Black Hole
DOI: 10.1086/187588 Bibcode: 1994ApJ...435L..35H

Kriss, Gerard A.; Hartig, George F.; Ford, Holland C. +7 more

Using the Faint Object Spectrograph on the Hubble Space Telescope (HST) to observe the central region of M87, we have obtained spectra covering ~4600-6800 A at a spectral dispersion ~4.4 A per resolution element through the 0.26" diameter entrance aperture. One spectrum was obtained centered on the nucleus of M87 and two centered 0.25" off the nuc…

1994 The Astrophysical Journal
eHST 361
Postrefurbishment Mission Hubble Space Telescope Images of the Core of the Orion Nebula: Proplyds, Herbig-Haro Objects, and Measurements of a Circumstellar Disk
DOI: 10.1086/174892 Bibcode: 1994ApJ...436..194O

O'Dell, C. R.; Wen, Zheng

We report on observations of M42 made with the Hubble Space Telescope (HST) immediately after the successful repair and refurbishment mission. Images were made in the strongest optical emission lines of H I, (N II), and (O III) and in a bandpass close to V. In a previous paper, the term proplyd was introduced to describe young stars surrounded by …

1994 The Astrophysical Journal
eHST 336
Narrowband HST Images of M87: Evidence for a Disk of Ionized Gas around a Massive Black Hole
DOI: 10.1086/187586 Bibcode: 1994ApJ...435L..27F

Kriss, Gerard A.; Bohlin, Ralph C.; Hartig, George F. +7 more

We present HST WFPC2 narrowband Hα + [N II] images of M87 which show a small disk of ionized gas with apparent spiral structure surrounding the nucleus of M87. The jet projects ~19.5^deg^ from the minor axis of the disk, which suggests that the jet is approximately normal to the disk. In a companion Letter, Harms et al. measure radial velocities a…

1994 The Astrophysical Journal
eHST 327
The Abundant Elements in Interstellar Dust
DOI: 10.1086/174438 Bibcode: 1994ApJ...430..650S

Savage, Blair D.; Sofia, Ulysses J.; Cardelli, Jason A.

We explore the incorporation of the cosmically abundant species O, C, N, Mg, Si, Fe, and S into interstellar dust. Column densities based on Goddard High Resolution Spectrograph 3.5 km/s resolution measurements from the literature for eight individual absorbing regions toward five lines of sight are used. Corrections are applied as needed in order…

1994 The Astrophysical Journal
eHST 263
HST Photometry of the Trapezium Cluster
DOI: 10.1086/173668 Bibcode: 1994ApJ...421..517P

Stauffer, John R.; Prosser, Charles F.; Hartmann, Lee +4 more

We have obtained images of 11 fields in the Trapezium cluster with the Planetary Camera (PC) of the Hubble Space Telescope (HST) in order to extend Herbig & Terndrup's (1986) study of this prototype, dense embedded cluster to fainter magnitudes than is possible from the ground. Using these images, we have identified 319 stars within an area of…

1994 The Astrophysical Journal
eHST 257
Morphological Studies of the Galaxy Populations in Distant ``Butcher-Oemler'' Clusters with HST. I. AC 114 at Z = 0.31 and Abell 370 at Z = 0.37
DOI: 10.1086/174387 Bibcode: 1994ApJ...430..121C

Smail, Ian; Ellis, Richard S.; Sharples, Ray M. +1 more

We present the first results of an ongoing program we are undertaking with the Wide Field Camera of the Hubble Space Telescope (HST) to understand the physical origin of the enhanced star formation seen in moderate-redshift (z ~ 0.3-0.4) cluster galaxies. Deep HST exposures have been obtained for the central regions of two rich compact "Butcher- O…

1994 The Astrophysical Journal
eHST 228
Hubble Space Telescope Imaging of Super--Star Clusters in NGC 1569 and NGC 1705
DOI: 10.1086/174625 Bibcode: 1994ApJ...433...65O

O'Connell, Robert W.; Gallagher, John S., III; Hunter, Deidre A.

We examine the structural properties of three super-star clusters in the nearby, H I-rich galaxies NGC 1569 and NGC 1705. The clusters, which have total absolute V magnitudes between - 13.3 and - 14.1, appear to be point sources on ground-based images but are partially resolved in new images obtained with the Hubble Space Telescope (HST) Planetary…

1994 The Astrophysical Journal
eHST 222
The Morphology of Distant Cluster Galaxies. I. HST Observations of CL 0939+4713
DOI: 10.1086/174386 Bibcode: 1994ApJ...430..107D

Dressler, Alan; Oemler, Augustus, Jr.; Butcher, Harvey R. +1 more

We have obtained Hubble Space Telescope (HST) WFC observations of CL 0939+4713, a very rich cluster at z = 0.41 which exhibits an excess population of blue galaxies typical of clusters at that redshift. The images are of sufficient quality, despite the HST spherical aberration problems, to permit assignment of Hubble types to galaxies brighter tha…

1994 The Astrophysical Journal
eHST 215
Steps toward Determination of the Size and Structure of the Broad-Line Region in Active Galactic Nuclei. V. Variability of the Ultraviolet Continuum and Emission Lines of NGC 3783
DOI: 10.1086/174007 Bibcode: 1994ApJ...425..582R

Altieri, B.; Mazeh, T.; Shull, J. M. +61 more

We report on the results of intensive ultraviolet spectral monitoring of the Seyfert 1 galaxy NGC 3783. The nucleus of NGC 3783 was observed with the International Ultraviolet Explorer satellite on a regular basis for a total of 7 months, once every 4 days for the first 172 days and once every other day for the final 50 days. Significant variabili…

1994 The Astrophysical Journal
IUE eHST 168