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2009•UvA-DARE (University of Amsterdam)Requires access

RXTE detects 245 Hz X-ray pulsations from IGR J17511-305

Craig B. Markwardt, D. Altamirano, Jean H. Swank, Tod E. Strohmayer, M. Linares, D. Pereira

Open publisher page 3 citations

Abstract

RXTE PCA Bulge scans detected activity of what appeared to be a known source. However, based on the results presented below, and the report of a new INTEGRAL source IGR J17511-305 (Baldovin et al. ATEL #2196), the activity detected by RXTE is due to a new 245 Hz X-ray pulsar.

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What this paper is about

RXTE PCA Bulge scans detected activity of what appeared to be a known source. However, based on the results presented below, and the report of a new INTEGRAL source IGR J17511-305 (Baldovin et al. ATEL #2196), the activity detected by RXTE is due to a new 245 Hz X-ray pulsar.

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OpenAlex reports 3 citations for this work. Citation counts describe recorded attention and do not establish research quality.

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Available abstract

RXTE PCA Bulge scans detected activity of what appeared to be a known source. However, based on the results presented below, and the report of a new INTEGRAL source IGR J17511-305 (Baldovin et al. ATEL #2196), the activity detected by RXTE is due to a new 245 Hz X-ray pulsar.

Key concepts: Physics, Pulsar, Astrophysics, Bulge, X-ray, Optics, Stars

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