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相关论文: Spitzer Observations of Tidal Dwarf Galaxies

200 篇论文

I discuss constraints on star formation and AGN in massive, red galaxies at z~1-3 using Spitzer observations at 3-24 micron. In particular I focus on a sample of distant red galaxies (DRGs) with J - K > 2.3 in the southern Great…

天体物理学 · 物理学 2007-05-23 Casey Papovich , GOODS , MIPS GTO teams

We use smoothed particle hydrodynamics (SPH) models to study the large-scale morphology and dynamical evolution of the intergalactic gas in Stephan's Quintet, and compare to multiwavelength observations. Specifically, we model the formation…

宇宙学与河外天体物理 · 物理学 2009-08-26 Jeong-Sun Hwang , Curtis Struck , Florent Renaud , Philip N. Appleton

We conduct spectral observations of 138 superthin galaxies (STGs) with high radial-to-vertical stellar disk scales ratio with the Dual Imaging Spectrograph (DIS) on the 3.5m telescope at the Apache Point Observatory (APO) to obtain the…

星系天体物理 · 物理学 2021-06-30 Dmitry Bizyaev , D. I. Makarov , V. P. Reshetnikov , A. V. Mosenkov , S. J. Kautsch , A. V. Antipova

In order to investigate the properties of the prominent tidal debris feature extending to the northeast of the compact group of galaxies Seyfert's Sextet, we analyzed multi-band (U, B, V, VR, R, I, J, H and K') photometric imaging data and…

天体物理学 · 物理学 2015-06-24 S. Nishiura , Y. Shioya , T. Murayama , Y. Sato , T. Nagao , Y. Taniguchi , D. B. Sanders

We present measurements of 5-25 {\mu}m emission features of brightest cluster galaxies (BCGs) with strong optical emission lines in a sample of 9 cool-core clusters of galaxies observed with the Infrared Spectrograph on board the Spitzer…

We examine the infrared properties of five low surface brightness galaxies (LSBGs) and compare them with related but higher surface brightness galaxies, using Spitzer Space Telescope images and spectra. All the LSBGs are detected in the 3.6…

We have carried out a detailed modelling of the dust heating and emission in the nearby, starbursting dwarf galaxy NGC 4214. Due to its proximity and the great wealth of data from the UV to the millimeter range (from GALEX, HST, {\it…

宇宙学与河外天体物理 · 物理学 2015-06-03 U. Lisenfeld , I. Hermelo , M. Relano , R. Tuffs , J. Fischera , B. Groves , C. Popescu

Recent observations have shown the presence of dust and molecular material in galactic winds, but relatively little is known about the distribution of these outflow components. To shed some light on this issue, we have used IRAC images from…

宇宙学与河外天体物理 · 物理学 2013-07-25 Alexander McCormick , Sylvain Veilleux , David S. N. Rupke

We present the results of a comprehensive Spitzer survey of 70 radio galaxies across 1<z<5.2. Using IRAC, IRS and MIPS imaging we determine the rest-frame AGN contribution to the stellar emission peak at 1.6um. The stellar luminosities are…

天体物理学 · 物理学 2019-08-15 N. Seymour , D. Stern , C. De Breuck

We present new Spitzer/IRAC observations of 55 dusty Long Period Variables (LPVs, 48 AGB and 6 RSG stars) in the Galaxy that have different chemistry, variability type, and mass-loss rate. O-rich AGB stars (including intrinsic S-type) tend…

太阳与恒星天体物理 · 物理学 2015-06-23 Megan Reiter , Massimo Marengo , Joseph L. Hora , Giovanni G. Fazio

We present mid-infrared spectra of 5 submillimeter galaxies at z=0.65-2.38 taken with the Spitzer Space Telescope. Four of these sources, at z<1.5, have strong PAH features and their composite spectrum is well fitted by an M82-like spectrum…

On the basis of observations by Spitzer and Herschel, we present and analyse the correlations between various monochromatic infrared (IR) luminosities for star-forming galaxies, selected from two northern Spitzer Wide-area InfraRed…

星系天体物理 · 物理学 2015-06-23 Yi-Nan Zhu , Hong Wu

Spitzer Infrared Spectrograph (IRS) observations of 3C radio galaxies and quasars shed new light on the nature of the central engines of AGN. Emission from silicate dust obscuring the central engine can be used to estimate the bolometric…

天体物理学 · 物理学 2007-05-23 P. M. Ogle , R. R. J. Antonucci , D. Whysong

Optical spectroscopic observations of white dwarf stars selected from catalogs based on the Gaia DR2 database reveal nine new gaseous debris disks that orbit single white dwarf stars, about a factor of two increase over the previously known…

太阳与恒星天体物理 · 物理学 2020-12-23 Carl Melis , B. Klein , A. E. Doyle , A. J. Weinberger , B. Zuckerman , P. Dufour

The atmospheres of very cool, hydrogen-rich white dwarfs (Teff <6000 K) are challenging to models because of the increased complexity of the equation of state, chemical equilibrium, and opacity sources in a low-temperature, weakly ionized…

太阳与恒星天体物理 · 物理学 2015-06-22 D. Saumon , J. B. Holberg , P. M. Kowalski

Using the Infrared Spectrograph on the Spitzer Space Telescope, we observed the Antennae galaxies obtaining spectral maps of the entire central region and high signal-to-noise 5-38 um spectra of the two galactic nuclei and six…

We present Spitzer high-resolution spectra of off-nuclear regions in the central cluster galaxies NGC 1275 and NGC 4696 in the Perseus and Centaurus clusters, respectively. Both objects are surrounded by extensive optical emission-line…

天体物理学 · 物理学 2009-11-13 R. Johnstone , N. Hatch , G. Ferland , A. Fabian , C. Crawford , R. Wilman

We present the first mid-infrared Spitzer/Infrared Spectrograph (IRS) observations of powerful radio galaxies at z>2. These radio galaxies, 4C +23.56 (z=2.48) and 6C J1908+7220 (z=3.53), both show strong mid-infrared continua, but with 6C…

天体物理学 · 物理学 2009-11-13 N. Seymour , P. Ogle , C. De Breuck , G. G. Fazio , A. Galametz , M. Haas , M. Lacy , A. Sajina , D. Stern , S. P. Willner , J. Vernet

We present new follow-up observations of two ultra-diffuse galaxies (UDGs) selected for their distorted morphologies and tidal features, suggestive of tidal influence. Using Hubble Space Telescope Advanced Camera for Surveys F555W and F814W…

Herbig Ae/Be stars are a class of young pre-main sequence stellar objects of intermediate mass and are known to have varying amounts of natal cloud material still present in their direct vicinity. We characterise the IR emission bands, due…