THE BALMER-DOMINATED BOW SHOCK AND WIND NEBULA STRUCTURE OF gamma-RAY PULSAR PSR J1741-2054
We have detected an Hα bow shock nebula around PSR J1741-2054, a pulsar discovered through its GeV γ-ray pulsations. The pulsar is only ∼1'.5 behind the leading edge of the shock. Optical spectroscopy shows that the nebula is non-radiative, dominated by Balmer emission. The Hα images and spectr...
Päätekijät: | Romani, R, Shaw, MS, Camilo, F, Cotter, G, Sivakoff, G |
---|---|
Aineistotyyppi: | Journal article |
Kieli: | English |
Julkaistu: |
2010
|
Samankaltaisia teoksia
-
17.41 Introduction to International Relations, Spring 2018
Tekijä: Hayes, Jarrod
Julkaistu: (2023) -
A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
Tekijä: Chakrabarty, Deepto
Julkaistu: (2020) -
LMXB AND IMXB EVOLUTION: I. THE BINARY RADIO PULSAR PSR J1614–2230
Tekijä: Lin, Jinrong, et al.
Julkaistu: (2015) -
LMXB and IMXB Evolution: I. The Binary Radio Pulsar PSR J1614-2230
Tekijä: Lin, J, et al.
Julkaistu: (2011) -
MeerKAT discovery of radio emission from the Vela X-1 bow shock
Tekijä: van den Eijnden, J, et al.
Julkaistu: (2021)