NGC 7582: The Prototype Narrow-Line X-Ray Galaxy

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

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

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The 10 – 200 μ m spectral energy distribution of the prototype narrow - line X - ray galaxy NGC 7582 ?

We present the spectral energy distribution (SED) between 10 and 200 μm obtained for the prototype narrowline X-ray galaxy NGC 7582 with ISOPHOT, the photometer on board the Infrared Space Observatory. The emission is spatially extended and we separated for the first time the nuclear and extranuclear infrared SEDs. The nuclear luminosity (LIR ∼ 4.5 × 1010 L ) is dominated by cold (T ∼ 32 K) dus...

متن کامل

Broad Band X-ray Observations of the Narrow Line X-ray Galaxy

We present a detailed analysis of broad band X-ray data of the Seyfert 2 galaxy NGC5506, obtained with the ASCA and ROSAT, to address the nature of Fe Kα line profile and the soft X-ray excess in this AGN. Variations up to 60% in the 2-10 keV band are detected during a 1-day ASCA observation performed in January 1997, while no significant change in the 2-10 keV continuum shape is found. The ASC...

متن کامل

X - RAY SPECTROSCOPY OF THE Fe K LINE IN THE SEYFERT 1 GALAXY NGC 3783

We report on the results of detailed X-ray spectroscopy of the Fe-K region in the Seyfert 1 galaxy NGC 3783 using the Chandra High Energy Grating Transmission Spectrometer (HETGS). There were five observations over an interval of ∼ 125 days in 2001, each with an exposure time of ∼ 170 ks. The combined data constitute the highest signal-to-noise Fe-K spectrum having the best velocity resolution ...

متن کامل

X - ray emission from the Sculptor galaxy NGC 300

We report here the results of a full analysis of all the ROSAT PSPC spectral imaging observations and all the ROSAT HRI high resolution imaging observations of the very nearby (D = 2.1 Mpc) Sculptor galaxy, NGC 300. Many point sources are detected within the field, several of them showing evidence for variability, and we present full source lists detailing their X-ray properties, and attempt to...

متن کامل

The X - Ray È Faint Early - Type Galaxy Ngc 4697

We analyze archival ROSAT HRI, ROSAT PSPC, and ASCA data of the X-rayÈfaint early-type galaxy NGC 4697. The joint ROSAT PSPC]ASCA spectrum is Ðtted by a two-component thermal model, a MEKAL model with keV with low metallicity and a bremsstrahlung kT MEKAL \ 0.26 ~0.03 `0.04 model with keV. A similar model was found to Ðt the spectra of another faint earlykT BREM \ 5.2 ~1.6 `3.0 type galaxy (NGC...

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

ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 1998

ISSN: 0004-637X

DOI: 10.1086/311537