1997AIP conference proceedingsRequires access

Evolution of the orbital period of Her X–1: Determination of a new ephemeris using RXTE data

B. Stelzer, R. Staubert, J. Wilms, Ralf D. Geckeler, D. E. Gruber, R. E. Rothschild

Open publisher page 3 citations

Abstract

Her X–1 was observed by RXTE in July 1996 during the MAIN HIGH state of its 35 day cycle. Using data from the Proportional Counter Array (PCA) we redetermine the orbital parameters of the binary system. The analysis based on pulse-timing measurements yields new estimates for the orbital elements and an accurate spin period for the time of observation. By comparing our results with previous observations of Her X–1 we are able to report a new orbital ephemeris including an improved value for the decrease in orbital period.

About this research paper

What this paper is about

Her X–1 was observed by RXTE in July 1996 during the MAIN HIGH state of its 35 day cycle. Using data from the Proportional Counter Array (PCA) we redetermine the orbital parameters of the binary system. The analysis based on pulse-timing measurements yields new estimates for the orbital elements and an accurate spin period for the time of observation. By comparing our results with previous observations of Her X–1 we are able to report a new orbital ephemeris including an improved value for the decrease in orbital period.

Why it matters

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

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

Her X–1 was observed by RXTE in July 1996 during the MAIN HIGH state of its 35 day cycle. Using data from the Proportional Counter Array (PCA) we redetermine the orbital parameters of the binary system. The analysis based on pulse-timing measurements yields new estimates for the orbital elements and an accurate spin period for the time of observation. By comparing our results with previous observations of Her X–1 we are able to report a new orbital ephemeris including an improved value for the decrease in orbital period.

Key concepts: Ephemeris, Orbital period, Physics, Binary number, Orbital elements, Period (music), Astrophysics, Astronomy

Related papers

Back to paper searchBrowse research topicsOriginal source
Evolution of the orbital period of Her X–1: Determination of a new ephemeris using RXTE data — Research Paper | ScholarLens