16 citations
- California Institute of TechnologyUS7 papers
- Moscow Institute of Thermal TechnologyRU7 papers
- National Institute for AstrophysicsIT7 papers
- Stanford UniversityUS6 papers
- Princeton UniversityUS5 papers
- University of MichiganUS5 papers
- University of WashingtonUS5 papers
- Center for Astrophysics Harvard & SmithsonianUS4 papers
- CFA InstituteUS4 papers
- Columbia UniversityUS4 papers
- University of California, BerkeleyUS4 papers
- University of Wisconsin–MadisonUS4 papers
10 papers · 1 filter
Stellar population gradients in Seyfert 2 galaxies
Thaisa Storchi-Bergmann, Daniel I. Raimann, R. Gonzalez Delgado +4
We study the variation of the stellar population properties as a function of distance from the nucleus for a sample of 35 Seyfert 2 galaxies using the technique of stellar populati…
Automated object classification with ClassX
A. A. Suchkov, T. A. McGlynn, L. Angelini +13
ClassX is a project aimed at creating an automated system to classify X-ray sources and is envisaged as a prototype of the Virtual Observatory. As a system, ClassX integrates into…
FUSE Observations of the Post-AGB Star ZNG 1 in the Globular Cluster M5 (NGC 5904)
W. V. Dixon, T. M. Brown, W. B. Landsman
We have observed the hot post-AGB star ZNG 1 in the globular cluster M5 with the Far Ultraviolet Spectroscopic Explorer (FUSE). From the resulting spectrum, we derive an effective…
Observational Properties of Primordial Stellar Populations
N. Panagia, M. Stiavelli, H. C. Ferguson +1
We present the first results of a study of the expected properties of the first stellar generations in the Universe. In particular, we consider and discuss a series of properties t…
Probing Baryons in Galactic Halos and Gas Near Galaxies
K. R. Sembach, B. P. Wakker, B. D. Savage +2
We describe an extensive FUSE survey of highly ionized oxygen in the vicinity of the Milky Way that serves as an example of the type of study that would be desirable for other gala…
A New Formation Mechanism for the Hottest Horizontal-Branch Stars
Allen V. Sweigart, Thomas M. Brown, Thierry Lanz +2
Stars with very large mass loss on the red-giant branch can undergo the helium flash while descending the white-dwarf cooling curve. Under these conditions the flash convection zon…