Difference between revisions of "Geminga"
(→People involved) |
(→People involved) |
||
| Line 13: | Line 13: | ||
* Giulia Brunelli (giulia.brunelli@inaf.it) | * Giulia Brunelli (giulia.brunelli@inaf.it) | ||
* Rubén López-Coto (rlopezcoto@iaa.es) | * Rubén López-Coto (rlopezcoto@iaa.es) | ||
| + | * Giovanni Ceribella (ceribell@mpp.mpg.de) | ||
| + | * Paul K. H. Yeung (pkh91yg@icrr.u-tokyo.ac.jp) | ||
== Data available == | == Data available == | ||
* Wobble observations, offset = 0.4 deg | * Wobble observations, offset = 0.4 deg | ||
Revision as of 07:11, 16 October 2024
General information
- Name of the source: Geminga
- Brief description of the source: Radio-quiet middle-aged gamma-ray pulsar
- Object type : Pulsar
- Other relevant information: Third pulsar detected by IACTs
- RA: 06 33 54.15 (hh mm ss), Dec: +17 46 12.9 (dd mm ss)
- RA, Dec in deg (ICRS): 98.48 17.77
- Galactic coordinates: l=195.13 b=+04.27
People involved
- Álvaro Mas-Aguilar (alvmas@ucm.es)
- Marcos López-Moya (marcos@gae.ucm.es)
- Giulia Brunelli (giulia.brunelli@inaf.it)
- Rubén López-Coto (rlopezcoto@iaa.es)
- Giovanni Ceribella (ceribell@mpp.mpg.de)
- Paul K. H. Yeung (pkh91yg@icrr.u-tokyo.ac.jp)
Data available
- Wobble observations, offset = 0.4 deg
