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相关论文: Nearby Galaxies with Spitzer

200 篇论文

We are performing a systematic study of the properties of early-type galaxies in the mid infrared spectral region with the Spitzer Space Telescope. We present here high S/N Spitzer IRS spectra of 17 Virgo early-type galaxies. Thirteen…

天体物理学 · 物理学 2007-05-23 A. Bressan , P. Panuzzo , L. Silva , L. Buson , M. Clemens , G. L. Granato , R. Rampazzo , J. R. Valdes , O. Vega

We performed an analysis of the mid-infared properties of the 12micron Seyfert sample, a complete unbiased 12micron flux limited sample of local Seyfert galaxies selected from the IRAS Faint Source Catalog, based on low resolution spectra…

宇宙学与河外天体物理 · 物理学 2015-05-14 V. Charmandaris , Yanling Wu , J. Huang , L. Spinoglio , S. Tommasin

Roughly half of the radiation from evolving galaxies in the early universe reaches us in the far-infrared and submillimeter wavelength range. Recent major advances in observing capabilities, in particular the launch of the Herschel Space…

星系天体物理 · 物理学 2015-06-19 D. Lutz

We introduce a new infrared diagnostic to separate galaxies on the basis of their dominant infrared emission: stellar or nuclear. The main novelty with respect to existing diagnostics, is the usage of a broad band encompassing at the same…

星系天体物理 · 物理学 2015-06-22 Dario Fadda , Giulia Rodighiero

We have investigated the mid-infrared (MIR) and visual structures of seven bipolar planetary nebulae (BPNe), using imaging and spectroscopy acquired using the Spitzer Space Telescope (SST), and the Observatorio Astronomico Nacional in…

星系天体物理 · 物理学 2010-04-02 J. P. Phillips , G. Ramos-Larios

We present deep mid-infrared spectroscopy with the Spitzer Space Telescope of 13 submillimeter galaxies (SMGs) in the Great Observatories Origins Deep Survey North (GOODS-N) field. We find strong polycyclic aromatic hydrocarbon (PAH)…

In this paper we present Spitzer Infrared Spectrograph spectroscopy for 14 intermediate-mass young stellar objects. We use Spitzer spectroscopy to investigate the physical properties of these sources and their environments. Our sample can…

太阳与恒星天体物理 · 物理学 2015-05-30 Jan Pitann , Martin Hennemann , Stephan Birkmann , Jeroen Bouwman , Oliver Krause , Thomas Henning

We report on the first mid-infrared observations of 16 GRB host galaxies performed with the Spitzer Space Telescope, and investigate the presence of evolved stellar populations and dust-enshrouded star-forming activity associated with GRBs.…

天体物理学 · 物理学 2009-11-11 E. Le Floc'h , V. Charmandaris , W. J. Forrest , F. Mirabel , L. Armus , D. Devost

The determination of chemical abundances in star-forming galaxies and the study of their evolution on cosmological timescales are powerful tools for understanding galaxy formation and evolution. This contribution presents the latest results…

天体物理学 · 物理学 2007-05-23 Thierry Contini

We present mid-infrared spectra and photometry of thirteen redshift 0.4<z<1 dust-reddened quasars obtained with Spitzer IRS and MIPS. We compare properties derived from their infrared spectral energy distributions (intrinsic AGN luminosity…

宇宙学与河外天体物理 · 物理学 2012-09-27 Tanya Urrutia , Mark Lacy , Henrik Spoon , Eilat Glikman , Andreea Petric , Bernhard Schulz

Mid-infrared diagnostics are presented for a large portion of the Spitzer Infrared Nearby Galaxies Survey (SINGS) sample plus archival data from the Infrared Space Observatory and the Spitzer Space Telescope. Our main result is that these…

We present mid-infrared spectra and photometry from the Infrared Spectrograph on the Spitzer Space Telescope for 51 OH megamasers (OHMs), along with 15 galaxies confirmed to have no megamaser emission above L_OH = 10^2.3 L_sun. The majority…

宇宙学与河外天体物理 · 物理学 2015-05-27 Kyle W. Willett , Jeremy Darling , Henrik W. W. Spoon , Vassilis Charmandaris , Lee Armus

We report on our first results from a mid-infrared spectroscopic study of ISM features in a sample of deeply obscured ULIRG nuclei using the InfraRed Spectrograph (IRS) on the Spitzer Space Telescope. The spectra are extremely rich and…

天体物理学 · 物理学 2009-11-11 H. W. W. Spoon , J. V. Keane , J. Cami , F. Lahuis , A. G. G. M. Tielens , L. Armus , V. Charmandaris

Here we present new - and, nevertheless, last - mid-infrared (mid-IR) data for supernovae (SNe) based on measurements with the Spitzer Space Telescope. Comparing our recent 3.6 and 4.5 $\mu$m photometry with previously published mid-IR and…

The near- and mid-IR spectrum of many astronomical objects is dominated by emission bands due to UV-excited polycyclic aromatic hydrocarbons (PAH) and evaporating very small grains (eVSG). Previous studies with the ISO, Spitzer and AKARI…

星系天体物理 · 物理学 2015-10-12 Paolo Pilleri , Olivier Berné , Christine Joblin

Integral-field spectroscopy in the near-infrared (NIR) is a powerful tool to analyze the gaseous and stellar distributions and kinematics, as well as the excitation mechanisms in the centers of galaxies. The unique combination of NIR and…

星系天体物理 · 物理学 2015-11-11 Gerold Busch , Nastaran Fazeli , Semir Smajić , Andreas Eckart , Lydia Moser , Mónica Valencia-S.

We examine the UV reprocessing efficiencies of warm dust and polycyclic aromatic hydrocarbons (PAHs) through an analysis of the mid- and far-infrared surface luminosity densities of 85 nearby H$\alpha$-selected star-forming galaxies…

星系天体物理 · 物理学 2015-06-22 Jason E. Young , Caryl Gronwall , John J. Salzer , Jessica L. Rosenberg

High resolution mid-infrared spectra are presented for 155 nuclear and extranuclear regions from the Spitzer Infrared Nearby Galaxies Survey (SINGS). The fluxes for nine atomic forbidden and three molecular hydrogen mid-infrared emission…

Observations at far-infrared and submillimeter wavelengths promise to revolutionize the study of high redshift galaxies and AGN by providing a unique probe of the conditions within heavily extinguished regions of star formation and nuclear…

天体物理学 · 物理学 2009-10-31 David A. Neufeld

We present new images (groundbased optical and mid-infrared (MIR) from the Spitzer Space Telescope) and spectra (from Spitzer) of the archetypal starburst galaxy M 82. The Spitzer data show that the MIR emission extends at least 6 kpc along…