output
19952026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 1999 · astro-phShow all

56 papers · 2 filters

astro-ph1999★ 35 cited

CCD uvbyHbeta Photometry in Clusters: I. The Open Cluster Standard, IC 4651

B. J. Anthony-Twarog, B. A. Twarog

CCD photometry of the intermediate-age open cluster, IC 4651, on the uvbyHbeta system is presented and analyzed. By using a combination of the information from the color-magnitude…

astro-ph1999★ 30 cited

The Reappearance of the Transient Low Mass X-ray Binary X1658-298

Stefanie Wachter, Alan P. Smale, Charles Bailyn

In April 1999 the transient low mass X-ray binary X1658-298 resumed its strong and persistent X-ray emission after a 21-year interval of quiescence. We present RXTE data obtained s…

astro-ph1999★ 77 cited

The Neutral Hydrogen Distribution in Merging Galaxies: Differences between Stellar and Gaseous Tidal Morphologies

J. E. Hibbard, W. D. Vacca, M. S. Yun

We have mapped the neutral atomic gas (HI) in the three disk-disk merger systems NGC 520, Arp 220, and Arp 299. These systems differ from the majority of the mergers mapped in HI,…

astro-ph1999★ 65 cited

Calibration of Nebular Emission-Line Diagnostics: I. Stellar Effective Temperatures

M. S. Oey, M. A. Dopita, J. C. Shields +1

We present a detailed comparison of optical H II region spectra to photoionization models based on modern stellar atmosphere models. We examine both spatially resolved and integrat…

astro-ph1999★ 43 cited

The Butcher-Oemler Effect at Moderate Redshift

Anne J. Metevier, A. Kathy Romer, M. P. Ulmer

We present the results of Butcher-Oemler-style analysis of three moderate- redshift (0.1<z<0.2) clusters which have bimodal X-ray surface brightness profiles. We find that at least…

astro-ph1999★ 113 cited

Molecular Gas, Dust and Star Formation in the Barred Spiral NGC 5383

Kartik Sheth, Michael W. Regan, Stuart N. Vogel +1

We present multi-wavelength (interferometer and single-dish CO J=1-0, Halpha, broadband optical and near-infrared) observations of the classic barred spiral NGC 5383. We compare th…

astro-ph1999★ 49 cited

Identification of SH ro-vibrational lines in R And

I. Yamamura, K. Kawaguchi, S. T. Ridgway

We report the identification of SH ro-vibrational lines in the published high-resolution infrared spectrum of the S-type star, R And. This is the first astronomical detectio…

astro-ph1999★ 34 cited

Weak Gravitational Lensing by the Nearby Cluster Abell 3667

M. Joffre, P. Fischer, J. Frieman +6

We present two weak lensing reconstructions of the nearby () merging cluster Abell 3667, based on observations taken year apart under different seeing condit…

astro-ph1999★ 25 cited

Evidence for Large Scale Structure in the Lyman alpha Forest at z>2.6

G. M. Williger, A. Smette, C. Hazard +2

We present a search for spatial and redshift correlations in a 2 A resolution spectroscopic survey of the Lyman alpha forest at 2.15 < z < 3.37 toward ten QSOs concentrated within…

astro-ph1999★ 223 cited

A Spectroscopic Study of a Large Sample of Wolf-Rayet Galaxies

N. G. Guseva, Y. I. Izotov, T. X. Thuan

We analyze long-slit spectral observations of 39 Wolf-Rayet (WR) galaxies with heavy element mass fraction ranging over 2 orders of magnitude, from Zsun/50 to 2Zsun. Nearly all gal…

astro-ph1999★ 68 cited

A New Look At Carbon Abundances In Planetary Nebulae. IV. Implications For Stellar Nucleosynthesis

R. B. C. Henry, K. B. Kwitter, J. A. Bates

This paper is the fourth and final report on a project designed to study carbon abundances in a sample of planetary nebulae representing a broad range in progenitor mass and metall…

astro-ph1999★ 37 cited

The Distance to the LMC via the Eclipsing Binary HV 2274

C. A. Nelson, K. H. Cook, P. Popowski +1

We present UBV photometry of the eclipsing binary Harvard Variable 2274 in the Large Magellanic Cloud (LMC). The stellar parameters of this binary system were calculated by Guinan…

astro-ph1999★ 21 cited

Galactic Kinematics Towards the South Galactic Pole. First Results from the Yale-San Juan Southern Proper-Motion Program

René A. Méndez, Imants Platais, Terrence M. Girard +2

The predictions from a Galactic Structure and Kinematic model code are compared to the color counts and absolute proper-motions derived from the Southern Proper-Motion survey cover…

astro-ph1999★ 14 cited

The End of the Lines for OX 169: No Binary Broad-Line Region

J. P. Halpern, M. C. Eracleous

We show that unusual Balmer emission line profiles of the quasar OX 169, frequently described as either self-absorbed or double peaked, are actually neither. The effect is an illus…

astro-ph1999★ 61 cited

FIRST Bent-Double Radio Sources: Tracers of High-Redshift Clusters

E. L. Blanton, M. D. Gregg, D. J. Helfand +2

Bent-double radio sources can act as tracers for clusters of galaxies. We present imaging and spectroscopic observations of the environments surrounding ten of these sources (most…

astro-ph1999★ 130 cited

Keck Spectra of Brown Dwarf Candidates and a Precise Determination of the Lithium Depletion Boundary in the Alpha Persei Open Cluster

J. R. Stauffer, D. Barrado y Navascués, J. Bouvier +8

We have identified twenty-seven candidate very low mass members of the relatively young Alpha Persei open cluster from a six square degree CCD imaging survey. Based on their I magn…

astro-ph1999★ 87 cited

The Extraordinary `Superthin' Spiral Galaxy UGC7321. I. Disk Color Gradients and Global Properties from Multiwavelength Observations

L. D. Matthews, J. S. Gallagher, W. van Driel

We present B- and R-band imaging and photometry, H-alpha narrow-band imaging, NIR H-band imaging, and HI 21-cm spectroscopy of the nearby Sd spiral galaxy UGC7321. UGC7321 exhibits…

astro-ph1999★ 106 cited

The Unusual Infrared Object HDF-N J123656.3+621322

Mark Dickinson, Christopher Hanley, Richard Elston +11

We describe an object in the Hubble Deep Field North with very unusual near-infrared properties. It is readily visible in Hubble Space Telescope NICMOS images at 1.6um and from the…

astro-ph1999★ 81 cited

Abundance Analyses of Field RV Stars, V: DS Aquarii, UY Arae, TW Camelopardis, BT Librae, U Moncerotis, TT Ophiuchi, and RV Tauri

Sunetra Giridhar, David L. Lambert, Guillermo Gonzalez

Abundance analyses are presented and discussed for eight RV Tauri variables. The RV B star UY Ara shows the abundance anomalies seen in other RV B stars, namely elements that conde…

astro-ph1999★ 45 cited

The Luminous Type Ic SN 1992ar at z=0.145

Alejandro Clocchiatti, Mark M. Phillips, Nicholas B. Suntzeff +13

We present spectroscopic and photometric observations of SN1992ar, the more distant SN in the Calan/Tololo Survey. We compare its spectrum with those of nearby Type Ia and Ic SNe a…

astro-ph1999★ 63 cited

Spectrophotometry of HII Regions, Diffuse Ionized Gas and Supernova Remnants in M31: The Transition from Photo- to Shock-Ionization

V. C. Galarza, R. A. M. Walterbos, R. Braun

We present results of KPNO 4-m optical spectroscopy of discrete emission-line nebulae and regions of diffuse ionized gas (DIG) in M31. Long-slit spectra of 16 positions in the NE h…

astro-ph1999★ 109 cited

Evidence for Large-Scale Structure at z=2.4 From Lyman-alpha Imaging

William C. Keel, Seth H. Cohen, Rogier A. Windhorst +1

We present deep wide-field medium-band imaging in redshifted Lyman alpha of fields surrounding HST detections of faint emitters, to characterize their larger-scale environment. The…

astro-ph1999★ 29 cited

Spectroscopic Observations of Optically Selected Clusters of Galaxies from the Palomar Distant Cluster Survey

B. P. Holden, R. C. Nichol, A. K. Romer +4

We have conducted a redshift survey of sixteen cluster candidates from the Palomar Distant Cluster Survey (PDCS) to determine both the density of PDCS clusters and the accuracy of…

astro-ph1999★ 24 cited

Evolution in the Clustering of Galaxies for Z < 1

Robert J. Brunner, Andrew J. Connolly, Alex S. Szalay

Measuring the evolution in the clustering of galaxies over a large redshift range is a challenging problem. For a two-dimensional galaxy catalog, however, we can measure the galaxy…