Study of the long-term stability of two anomalous X-ray pulsars, 4U 0142+61 and 1E 1048.1-5937, with ASCA

We present new observations of two anomalous X-ray pulsars (AXPs), 4U 014261 and 1E 1048.1-5937, made in 1998 with ASCA. The energy spectrum of each of these two AXPs is found to consist of two components, a power-law and a blackbody emission from the neutron star surface. These observations, when compared with earlier ASCA observations in 1994, show remarkable stability in the intensities, spectral shapes, and pulse profiles. However, we find t hat the spin-down rate in 1E 1048.1-5937 is not constant. In this source, w e have clearly identified three epochs with spin-down rates different from each other and from the average value. This has very strong implications fo r the magnetar hypothesis for AXPs. We also note that the spin-down rate an d its variations in 1E 1048.1-5937 are much larger than can normally be pro duced by an accretion disk with a very low mass accretion rate correspondin g to its low X-ray luminosity.