SUMMARY OF PROPOSAL 71057
INSTITUTE OF SPACE AND ASTRONAUTICAL SCINECE
3-1-1 YOSHINODAI
SAGAMIHARA
KANAGAWA JAPAN 229-8510
Tel: 0427-59-8351 Fax: 0427-59-8455
Medium: 2.5GB8MM
Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION
IS RX J1838.4-0301 A MAGNETAR IN A SUPERNOVA REMNANT?
ABSTRACT
RX J1838.4-0301 is a point source in the supernova remnant (SNR) G28.8+1.5. A 5.45-s pulsation was found from the ROSAT observation and similarity of this system to the anomalous 6-s pulsar 1E2259+586/G109-1.0 system is proposed. However, there is an argumenet on the 6-s pulsar hypotesis of this pulsar. On the other hand, a hypotesis of a magnetar was proposed for the 1E 1841-045 /Kes 73 system which has properties similar to the above mentioned two systems. We propose ASCA observations of the RX J1838.4-0301/G28.8+1.5 system to confirm the 5.45-s pulsations of the source, to investigate the possibility of this source to be a magnetar, and to study the association of this source with the SNR.
CO-INVESTIGATORS
CO-I NAME | INSTITUTE | COUNTRY |
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MASANOBU OZAKI | ISAS | JAPAN |
MUTSUMI SUGIZAKI | ISAS | JAPAN |
JYUN'ICHI ISHIDA | ISAS | JAPAN |
MASAHIRO KAWASAKI | ISAS | JAPAN |
TARGETS
TARGET NAME | PRI | RA | DEC | TIME | TC | OFF | GIS | SIS CNT | OBS |
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1)RX J1838.4-0301 | B | 279.6121 | -3.0207 | 60 ks | N | Y | P | 0.01000 | 1 |
2)G28.8+1.5_WN | B | 279.5833 | -2.3444 | 20 ks | N | Y | P | 0.15000 | 1 |
3)G28.8+1.5_ES | B | 279.9167 | -2.6667 | 20 ks | N | Y | P | 0.15000 | 1 |