Universe  ID: 10798

Stellar Odd Couple Makes Striking Flares

Every 3.4 years, pulsar B1259-63 dives twice through the gas disk surrounding the massive blue star it orbits. With each pass, it produces gamma rays. During the most recent event, NASA's Fermi Gamma-ray Space Telescope observed that the pulsar's gamma-ray flare was much more intense the second time it plunged through the disk. Astronomers don't yet know why.

For the B1259 binary animation, go here.

 

Related


For More Information

http://www.nasa.gov/mission_pages/GLAST/news/odd-couple.html


Credits

Walt Feimer (HTSI): Lead Animator
Scott Wiessinger (USRA): Animator
Francis Reddy (SPSYS): Animator
Scott Wiessinger (USRA): Video Editor
Scott Wiessinger (USRA): Narrator
Scott Wiessinger (USRA): Producer
Aous Abdo (George Mason University): Scientist
Francis Reddy (SPSYS): Writer
Please give credit for this item to:
NASA/Goddard Space Flight Center. However, each image should be credited as indicated above.

Short URL to share this page:
http://svs.gsfc.nasa.gov/10798

Mission:
Fermi Gamma-ray Space Telescope

Data Used:
Fermi

This item is part of these series:
Narrated Movies
Astrophysics Stills
Astrophysics Features

Goddard TV Tape:
G2011-075 -- Odd Couple Binary

Keywords:
SVS >> Gamma Ray
SVS >> HDTV
SVS >> Neutron Star
SVS >> Astrophysics
SVS >> Pulsar
SVS >> Edited Feature
SVS >> Fermi
SVS >> Binary Star
DLESE >> Narrated
SVS >> Star
NASA Science >> Universe