• No results found

The isolated neutron star X ray pulsars RX J0420 0–5022 and RX J0806 4–4123 : new X ray and optical observations

N/A
N/A
Protected

Academic year: 2020

Share "The isolated neutron star X ray pulsars RX J0420 0–5022 and RX J0806 4–4123 : new X ray and optical observations"

Copied!
12
0
0

Loading.... (view fulltext now)

Full text

Loading

Figure

Table 1. Chandra ACIS and XMM-Newton EPIC observations.
Table 2. Black-body model fits to the EPIC-pn spectra obtained from individual observations.
Fig. 1. Merged EPIC-pn spectra of RX J0806.4 −4123 and RX J0420.0−5022 accumulated from all available observations
Fig. 2. RGS spectrum obtained by combining RGS1 and RGS2 spectra from the two observations of RX J0806.4 −4123
+5

References

Related documents

Orthopaedic oncology surgeons, musculoskeletal pathologists, bone radiologists, medical oncologists, reconstructive and reparative surgeons and medical radiation technologists

The goal of this approach would be twofold: on one hand, to define and provide a simple-to-interpret (but non-simplistic) tool to measure CMs development and integration between

How does an institutional perspective differ from contingency or open systems perspective in terms of the role of the environment and the mechanism through which the

From PC & web-based viewing and printing of documents in a wide range of formats, to professional color management, application drivers, touchscreen & cloud printing, KIP

conducting this study was to provide valuable information to the development of alternative ways to control air pollution from industries. b) To determine major

It was expected that the JET program would “provide increased opportunities for interaction in the schools between ALTs and Japanese teachers of foreign languages,” and through

channel designation which differs from that of the actual radio channel (or range of frequencies) on which the signal travels. The most common reason for a television station using