activity
19942023
most citedThe MACHO Project: Microlensing Results from 5.7 Years of LMC Observations

1k citations · 22.8k across the 263 of their papers we have counts for

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Showing 1999Show all

7 papers · 1 filter

astro-ph1999★ 9 cited

Intracluster Planetary Nebulae in the Virgo Cluster

K. C. Freeman, M. Arnaboldi, M. Capaccioli +8

We briefly describe the properties of the confirmed spectroscopic sample of intracluster planetary nebulae recently discovered in the Virgo cluster. We find 23 bonafide intracluste…

astro-ph1999★ 92 cited

New Galaxies Discovered in the First Blind HI Survey of the Centaurus A Group

G. D. Banks, M. J. Disney, P. M. Knezek +26

We have commenced a 21-cm survey of the entire southern sky (δ< 0 degrees, -1200 km/s < v < 12700 km/s) which is ''blind'', i.e. unbiased by previous optical information. In the pr…

astro-ph1999★ 7 cited

The HI and Ionized Gas Disk of the Seyfert Galaxy NGC 1144 = Arp 118: A Violently Interacting Galaxy with Peculiar Kinematics

M. A. Bransford, P. N. Appleton, C. F. McCain +1

We present observations of the distribution and kinematics of neutral and ionized gas in NGC 1144, a galaxy that forms part of the Arp 118 system. Ionized gas is present over a hug…

astro-ph1999★ 203 cited

The Formation and Evolution of Young Globular Clusters in NGC 3256

S. E. Zepf, K. M. Ashman, J. English +2

We present images of the recent galaxy merger NGC 3256 obtained with the WFPC2 of the Hubble Space Telescope in B and I filters. We show that there is a large population of more th…

astro-ph1999★ 227 cited

The Nature of Boxy/Peanut-Shaped Bulges in Spiral Galaxies

M. Bureau, K. C. Freeman

We present a systematic observational study of the relationship between bars and boxy/peanut-shaped (B/PS) bulges. We first review and discuss proposed mechanisms for their formati…

astro-ph1999★ 59 cited

Difference Image Analysis of Galactic Microlensing I. Data Analysis

C. Alcock, R. A. Allsman, D. Alves +18

This is a preliminary report on the application of Difference Image Analysis (DIA) to galactic bulge images. The aim of this analysis is to increase the sensitivity to the detectio…