Astrobiology Science News 3 February 2011
- Experiment reaches biology milestone with hard X-ray laser, ASU
- Laboratory Giant virus, tiny protein crystals show X-ray laser’s power and potential, SLAC
- Scientists Help NASA Find Earth-size Planet Candidates, UCSB
- UF astronomers, NASA team find six closely packed planets orbiting same star, University of Florida
- A Closely-Packed System of Low-Mass, Low-Density Planets Transiting Kepler-11 (full paper), astro-ph
- Accretion of a Terrestrial-Like Minor Planet by a White Dwarf, astro-ph
- Solar wind origin of terrestrial water, astro-ph
- Exoplanets around G-K Giants, astro-ph
- A Planet of an A-Star: HD15082b, astro-ph
- Planets around Extreme Horizontal Branch Stars, astro-ph
- Analysis of Two Eclipsing Hot Subdwarf Binaries with a Low Mass Stellar and a Brown Dwarf Companion
- , astro-ph
- A Planetary Companion around a Metal-Poor Star with Extragalactic Origin, astro-ph
- Brown Dwarf Companions to White Dwarfs, astro-ph
- Latest Results from the DODO Survey: Imaging Planets around White Dwarfs, astro-ph
- Searching for Planets with White Dwarf Pulsations: Spurious Detections, astro-ph
- The Planets around the Post-Common Envelope Binary NN Serpentis, astro-ph
- On the Origin of Metals in Some Hot White Dwarf Photospheres, astro-ph
- Study of Planetary Systems around Giant Stars, astro-ph
- Towards a New Prescription for the Tidal Capture of Planets, Brown Dwarfs and Stellar Companions, astro-ph
- Transit timing variations in the HAT-P-13 planetary system, astro-ph
- Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data, astro-ph
- Architecture and Dynamics of Kepler’s Candidate Multiple Transiting Planet Systems, astro-ph
- Transit Timing Observations from Kepler: I. Statistical Analysis of the First Four Months, astro-ph
- The Distribution of Transit Durations for Kepler Planet Candidates and Implications for their Orbital Eccentricities, astro-ph
- The atmospheres of the hot-Jupiters Kepler-5b and Kepler-6b observed during occultations with Warm-Spitzer and Kepler, astro-ph
