22 citations
- Berkeley CollegeUS5 papers
- California Institute of TechnologyUS5 papers
- Michigan Science CenterUS4 papers
- Lawrence Livermore National LaboratoryUS3 papers
- Vanderbilt HealthUS3 papers
- Vanderbilt UniversityUS3 papers
- Yale UniversityUS3 papers
- Association for Language LearningGB2 papers
- Moscow Institute of Thermal TechnologyRU2 papers
- Princeton Public SchoolsUS2 papers
- University of BonnDE2 papers
- University of California, BerkeleyUS2 papers
6 papers · 2 filters
Recent Breakthroughs in Detecting Neutron Star Binaries in Globular Clusters
Peter D. Edmonds
Binary stars have long been considered to play a crucial role in globular cluster evolution, and offer the advantages of studying systems at the same, well-determined distances. Ho…
Measuring the Influence of Supernovae at High Redshift
K. L. Adelberger
Supernovae play a large but poorly understood role in our attempts to explain the evolution of the baryonic universe. Numerous observations throughout astronomy cannot be explained…
Comment on "Chandra Reveals The X-ray Glint in the Cat's Eye"
H. L. Maness, S. D. Vrtilek
Chu et al (2001; ApJ, 533, L69) report that they find the diffuse X-ray emission from the Cat's Eye Nebula, NGC 6543, to be inconsistent with nebular abundances but consistent with…
Towards Proper Motions in the Local Group
A. Brunthaler, M. Reid, H. Falcke +2
Key and still largely missing parameters for measuring the mass content and distribution of the Local Group are the proper motion vectors of its member galaxies. The problem when t…
Probing the Initial Conditions of Clustered Star Formation -- Large Scale On-the-Fly Mapping of Orion B at FCRAO
Naomi A. Ridge, Edwin A. Bergin, S. T. Megeath
In order to obtain a census of the pre-stellar and star-forming molecular cores, we have begun an unbiased survey in CS and N2H+ of the L1630 and L1641 molecular clouds. The use of…
On the discrepancy between Chandra and XMM temperature profiles for A1835
Maxim Markevitch
This short technical note addresses a large discrepancy between the temperature profiles for the galaxy cluster A1835 derived by Schmidt et al. (2001) using Chandra and by Majerowi…