INTEGRAL observations of the peculiar BeX System SAX J 2103 . 5 + 4545

نویسندگان

  • P. Blay
  • P. Reig
  • S. Martı́nez Núñez
  • A. Camero
  • V. Reglero
چکیده

We present an INTEGRAL data analysis of the X-ray transient SAX J2103.5+4545 during two outbursts detected in December 2002. The INTEGRAL coordinates and error circle agree with the position of the recently proposed optical counterpart. A power-law plus cutoff model provided a good fit to the 4–150 keV spectrum yielding a photon index of 1.0±0.1, a cutoff energy E cut = 7.6 ± 2.0 keV and a folding energy E fold = 30.9 ± 2.5 keV. The X-ray luminosity in the 4-150 keV energy range was found to be 6.0×10 36 erg s −1 , assuming a distance of 6.5 kpc. This luminosity, together with the derived photon index, indicate that the source is in a bright state. A 354.9±0.5 second pulse period is measured. This value is significantly smaller than previous measurements, indicating a long-term spin-up episode.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

A large spin – up rate measured with INTEGRAL in the High Mass X – ray Binary Pulsar SAX J 2103 . 5 + 4545

The High Mass X–ray Binary Pulsar SAX J2103.5+4545 has been observed with INTEGRAL several times during the last outburst in 2002–2004. We report a comprehensive study of all INTEGRAL observations, allowing a study of the pulse period evolution during the recent outburst. We measured a very rapid spin-up episode, lasting ∼130 days, which decreased the pulse period by ∼1.8 s. The spin-up rate, Ṗ...

متن کامل

Discovery of the transient X - ray pulsar SAX J 2103 . 5 + 4545

We report the discovery of the X-ray transient SAX J2103.5+4545 which was active from Febru-ary to September 1997. The observed peak intensity of 20 mCrab (2 to 25 keV) occurred on April 11. An analysis of data obtained around the time of the peak revealed a pulsed signal with a period of 358.61 ± 0.03 s on MJD 50569. The pulse profile has a pulsed fraction of ∼ 40%. No change in the pulse peri...

متن کامل

Long-term pulse profile study of the Be/X-ray pulsar SAX J2103.5+4545

Aims. We present the first long-term pulse profile study of the X-ray pulsar SAX J2103.5+4545. Our main goal is to study the pulse shape correlation either with luminosity, time or energy. Methods. This Be/X-ray binary system was observed from 1999 to 2004 by RXTE PCA, and by INTEGRAL from 2002 to 2005, during the Performance and Verification (PV) phase and the Galactic Plane Scan survey (GPS)....

متن کامل

Identification of the optical counterparts of high-mass X-ray binaries through optical photometry and spectroscopy

We present the results of our search for optical counterparts to high-mass X-ray transient sources discovered by various X-ray missions. We obtained CCD images of the X-ray fields through BVR and Hα filters in order to identify early-type stars in the R − Hα versus B − V colour-colour diagram. We also obtained medium-resolution spectroscopy of the candidates in order to confirm the presence of ...

متن کامل

Discovery of a 30 day period in the supergiant fast X - ray transient SAX J 1818 . 6 − 1703

SAX J1818.6−1703 has been characterised as a Supergiant Fast X-ray Transient system on the basis of several INTEGRAL/IBIS detections since the original BeppoSAX Wide Field Camera detection. Using IBIS/ISGRI, Swift/BAT and archival observations, we show that in fact SAX J1818.6−1703 exhibits emission on a period of 30 ± 0.1 days, with a high degree of recurrence. SAX J1818.6−1703 is therefore th...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2004