High resolution infrared imaging and spectroscopy of the Pistol Nebula: evidence for ejection

نویسندگان

  • Donald Figer
  • Mark Morris
  • Thomas Geballe
  • Donald F. Figer
  • T. R. Geballe
  • R. Michael Rich
  • Eugene Serabyn
  • Ian S. McLean
  • R. C. Puetter
  • Amos Yahil
چکیده

We present new infrared images, obtained with the Hubble Space Telescope (HST) Near-infrared Camera and Multi-object Spectrometer (NICMOS), and Br-α (4.05 μm) spectroscopy, obtained using CGS4 on UKIRT, of the Pistol Star and its associated nebula. We find strong evidence to support the hypothesis that the Pistol Nebula was ejected from the Pistol Star. The Pa-α (1.87 μm) NICMOS image shows that the nebula completely surrounds the Pistol Star, although the line intensity is much stronger on its northern and western edges. The Br-α CGS4 spectra show the classical ring-like signature of quasi-spherical expansion. The blueshifted emission (Vmax ≈ −60 km s ) is much weaker than the redshifted emission (Vmax ≈ +10 km s ), where the velocities are with respect to the velocity of the Pistol Star; further, the redshifted emission spans a very narrow range of velocities, i.e., it appears “flattened” in the Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract No. NAS5-26555. Division of Astronomy, Department of Physics & Astronomy, University of California, Los Angeles, 405 Hilgard Avenue, Los Angeles, CA 90095-1562; [email protected], [email protected], [email protected], [email protected] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 Gemini Observatory, 670 N. A’ohoku Place, Hilo, HI 96720; [email protected] JPL 171-113, 4800 Oak Grove Dr., Pasadena, CA 91109; [email protected] Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive, La Jolla, CA 92093-0111; [email protected] Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, NY 11794-3800; [email protected] Institut d’Astrophysique de Paris, 98 bis Blvd Arago, 75014 Paris, France

برای دانلود رایگان 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

ar X iv : a st ro - p h / 99 06 47 9 v 1 2 9 Ju n 19 99 High Resolution Infrared Imaging and Spectroscopy of the Pistol Nebula : Evidence for Ejection 1 Donald

We present new infrared images, obtained with the Hubble Space Telescope (HST) Near-infrared Camera and Multi-object Spectrometer (NICMOS), and Br-α (4.05 μm) spectroscopy, obtained using CGS4 on UKIRT, of the Pistol Star and its associated nebula. We find strong evidence to support the hypothesis that the Pistol Nebula was ejected from the Pistol Star. The Pa-α (1.87 μm) NICMOS image shows tha...

متن کامل

High Resolution Infrared Imaging and Spectroscopy of the Pistol Nebula: Evidence for Ejection1

We present new infrared images, obtained with the Hubble Space Telescope (HST) Near-infrared Camera and Multi-object Spectrometer (NICMOS), and Br-α (4.05 μm) spectroscopy, obtained using CGS4 on UKIRT, of the Pistol Star and its associated nebula. We find strong evidence to support the hypothesis that the Pistol Nebula was ejected from the Pistol Star. The Pa-α (1.87 μm) NICMOS image shows tha...

متن کامل

High - resolution imaging of the bipolar nebula Red Rectangle Evidence for unstable mass transfer in a close binary system ?

We present the first diffraction-limited specklemasking bispectrum observations of the central part of the Red Rectangle at optical wavelengths (λ ∼ 656 nm and λ ∼ 800 nm). The results confirm infrared observations which show that the object is a bipolar nebula. The dark lane separating the two lobes is probably produced by an obscuring dust disk slightly inclined with respect to the line of si...

متن کامل

1 5 Ju n 20 09 High Angular Resolution Imaging Spectroscopy of the Galactic Ultra – Compact H II Region K 3 – 50 A

Gemini North adaptive optics imaging spectroscopy is presented for the Galactic ultra–compact H II (UCH II) region K3–50A. Data were obtained in the K−band using the Near–infrared Integral Field Spectrograph (NIFS) behind the facility adaptive optics module ALTAIR in natural guide star mode. The NIFS data cube reveals a complex spatial morphology across the 0.1 pc scale of the 3 UCH II region. ...

متن کامل

Performance of myocardial perfusion imaging using multi-focus fan beam collimator with resolution recovery reconstruction in a comparison with conventional SPECT

  Objective: IQSPECT is an advanced high-speed SPECT modality for performing myocardial perfusion imaging (MPI), which uses a multi-focus fan beam collimator with resolution recovery reconstruction. The aim of this study was to compare IQSPECT compared with conventional SPECT interms of performance based on standard clinical protocols. In addition, we examined the concordance between convention...

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

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2016