ar X iv : a st ro - p h / 05 07 22 1 v 1 8 J ul 2 00 5 A Radio Transient 0 . 1 pc from Sagittarius A *
نویسندگان
چکیده
We report the discovery of a transient radio source 2.7 arcsec (0.1 pc projected distance) South of the Galactic Center massive black hole, Sagittarius A*. The source flared with a peak of at least 80 mJy in March 2004. The source was resolved by the Very Large Array into two components with a separation of ∼ 0.7 arcsec and characteristic sizes of ∼ 0.2 arcsec. The two components of the source faded with a power-law index of 1.1± 0.1. We detect an upper limit to the proper motion of the Eastern component of ∼ 3× 10 km s relative to Sgr A*. We detect a proper motion of ∼ 10 km s for the Western component relative to Sgr A*. The transient was also detected at X-ray wavelengths with the Chandra X-ray Observatory and the XMM-Newton telescope and given the designation CXOGC J174540.0-290031. The X-ray source falls in between the two radio components. The maximum luminosity of the X-ray source is ∼ 10 erg s, significantly sub-Eddington. The radio jet flux density predicted by the X-ray/radio correlation for X-ray binaries is orders of magnitude less than the measured flux density. We conclude that the radio transient is the result of a bipolar jet originating in a single impulsive event from the X-ray source and interacting with the dense interstellar medium of the Galactic Center. Subject headings: Galaxy: center — ISM: jets and outflows — radio continuum: general — X-rays: binaries Astronomy Department & Radio Astronomy Laboratory, University of California, Berkeley, CA 94720; gbower,dbacker,[email protected] Adler Planetarium and Astronomy Museum, 1300 South Lake Shore Drive, Chicago, IL 60605 Department of Physics and Astronomy, Northwestern University, Evanston, IL 60208; dougroberts,[email protected] National Radio Astronomy Observatory, Charlottesville, VA 22903; [email protected] National Radio Astronomy Observatory, P.O. Box O, Socorro, NM 87801; [email protected] Department of Physics and Astronomy, University of Iowa, 203 Van Allen Hall, Iowa City, IA 52245; [email protected]
منابع مشابه
ar X iv : a st ro - p h / 05 07 06 6 v 1 4 J ul 2 00 5 Multiband Echo Tomography of Sco X - 1
متن کامل
ar X iv : a st ro - p h / 00 07 10 5 v 1 8 J ul 2 00 0 THE BROAD BAND SPECTRUM AND VARIABILITY OF SEYFERT 1
Recent results on the X–ray spectrum and variability of Seyfert 1 galaxies are reviewed. New spectral results from BeppoSAX observations are also presented and briefly discussed.
متن کاملar X iv : a st ro - p h / 05 07 15 8 v 1 7 J ul 2 00 5 Asteroids . From Observations to Models
We will discuss some specific applications to the rotation state and the shapes of moderately large asteroids, and techniques of observations putting some emphasis on the HST/FGS instrument.
متن کاملar X iv : a st ro - p h / 05 07 14 5 v 1 6 J ul 2 00 5 X - ray Pulsations in the Supersoft X - ray Binary CAL 83
Received ; accepted – 2 – ABSTRACT Chandra and XMM-Newton X-ray data reveal that the supersoft X-ray binary CAL 83 exhibits 38.4 minute pulsations at some epochs. These X-ray variations are similar to those found in some novae and are likely to be caused by nonradial pulsations the white dwarf. This is the first detection of pulsations in a persistent supersoft source.
متن کاملar X iv : a st ro - p h / 01 05 53 8 v 1 3 0 M ay 2 00 1 Circumnuclear stellar population , morphology and environment of Seyfert 2 galaxies : an evolutionary scenario
We investigate the relation between the characteristics of the circumnuclear stellar population and both the galaxy morphology and the presence of close companions for a sample of 35 Seyfert 2 nuclei. Fifteen galaxies present unambiguous signatures of recent episodes of star formation within ≈300 pc from the Jansky Fellow Gemini Fellow
متن کامل