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Related papers: The Age-Dependence of Mid-Infrared Emission Around…

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Context. Spitzer Space Telescope observations and dust emission models are used to discuss the distribution of dust and its characteristics in M31. Together with GALEX FUV, NUV, and SDSS images we studied the age dependence of the dust…

Astrophysics of Galaxies · Physics 2015-05-13 M. Montalto , S. Seitz , A. Riffeser , U. Hopp , C. -H. Lee , R. Schönrich

We present a catalogue of 99 candidate clusters and groups of galaxies in the redshift range 0.1 < z_{phot} < 1.3 discovered in the Spitzer First Look Survey (FLS). The clusters are selected by their R - 3.6um galaxy color-magnitude…

Astrophysics · Physics 2009-11-13 Adam Muzzin , Gillian Wilson , Mark Lacy , H. K. C. Yee , S. A. Stanford

We present a study of the spatial distribution of the stellar cluster populations in the star forming galaxy NGC 628. Using Hubble Space Telescope broad band WFC3/UVIS UV and optical images from the Treasury Program LEGUS (Legacy…

Dust in Early-Type galaxies (ETGs) may originate from internal or external sources. In this paper we study the stellar populations of particularly dusty ETGs to search for evidence of the dust's origin. Using the Southern African Large…

Astrophysics of Galaxies · Physics 2026-04-08 Ron W. Savage , Anne E. Sansom , David H. W. Glass

It is often argued that young stellar clusters suffer a significant infant mortality that is partly related to the expulsion of dust and gas in their early phases caused by radiation pressure from hot stars and supernovae. Near-infrared…

Cosmology and Nongalactic Astrophysics · Physics 2013-03-11 P. Grosboel , H. Dottori

We compare star formation in the inner and outer disks of 11 dwarf Irregular galaxies (dIm) within 3.6 Mpc. The regions are identified on GALEX near-UV images, and modeled with UV, optical, and near-IR colors to determine masses and ages. A…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Nicholas W. Melena , Bruce G. Elmegreen , Deidre A. Hunter , Lea Zernow

The relationship between star formation and infrared emission in galaxies will be investigated. If galaxies were simple objects and young stars were completely covered with dust, then all the absorbed light of the young stars would be…

Astrophysics · Physics 2023-03-08 Nikolaos D. Kylafis , Angelos Misiriotis

We analyze very deep IRAC and MIPS photometry of $\sim$ 12,500 members of the 14 Myr old Double Cluster, h and $\chi$ Persei, building upon on our earlier, shallower Spitzer studies (Currie et al. 2007a, 2008a). Numerous likely members show…

Solar and Stellar Astrophysics · Physics 2015-06-22 Ryan Cloutier , Thayne Currie , George Rieke , Scott J. Kenyon , Zoltan Balog , Ray Jayawardhana

Although photometric and spectroscopic surveys with the Spitzer Space Telescope increased remarkably the number of well studied debris disks around A-type and Sun-like stars, detailed analyzes of debris disks around F-type stars remained…

Solar and Stellar Astrophysics · Physics 2015-05-20 A. Moór , I. Pascucci , Á. Kóspál , P. Ábrahám , T. Csengeri , L. L. Kiss , D. Apai , C. Grady , Th. Henning , Cs. Kiss , D. Bayliss , A. Juhász , J. Kovács , T. Szalai

We present evidence that the 8 $\mu$m (dust) and 24 $\mu$m luminosities of star-forming galaxies are both strongly correlated with their 1.4 GHz and H$\alpha$ luminosities over a range in luminosity of two-to-three orders of magnitude. At…

Astrophysics · Physics 2009-11-11 H. Wu , C. Cao , C. -N. Hao , F. -S. Liu , J. -L. Wang , X. -Y. Xia , Z. -G. Deng , C. -K. -S. Young

Recent interferometric surveys of nearby main-sequence stars show a faint but significant near-infrared excess in roughly two dozen systems, i.$\,$e. around $10\,\%$ to $30\,\%$ of stars surveyed. This excess is attributed to dust located…

Solar and Stellar Astrophysics · Physics 2017-02-01 Florian Kirchschlager , Sebastian Wolf , Alexander V. Krivov , Harald Mutschke , Robert Brunngräber

We have searched for infrared excesses around a well defined sample of 69 FGK main-sequence field stars. These stars were selected without regard to their age, metallicity, or any previous detection of IR excess; they have a median age of…

Astrophysics · Physics 2009-11-13 G. Bryden , C. A. Beichman , D. E. Trilling , G. H. Rieke

We present an analysis of wind-blown, parsec-sized, mid-infrared bubbles and associated star-formation using GLIMPSE/IRAC, MIPSGAL/MIPS and MAGPIS/VLA surveys. Three bubbles from the Churchwell et al. (2006) catalog were selected. The…

We have observed a sample of 35 long-period variables and four Cepheid variables in the vicinity of 23 Galactic globular clusters using the Infrared Spectrograph on the Spitzer Space Telescope. The long-period variables in the sample cover…

To investigate the nature of starbursts' dust, we constructed a model of the stars and dust in starburst galaxies and applied it to 30 observed starburst spectral energy distributions (SEDs). The starburst model was constructed by combining…

Astrophysics · Physics 2008-11-26 K. D. Gordon , D. Calzetti , A. N. Witt

We find that the initial dust masses in planetary debris disks are correlated with the metallicities of their central stars. We compiled a large sample of systems, including Spitzer, the Herschel DUNES and DEBRIS surveys, and WISE debris…

Solar and Stellar Astrophysics · Physics 2016-08-17 Andras Gaspar , George H. Rieke , Nicholas Ballering

We report the results of a spectroscopic search for debris disks surrounding 41 nearby solar type stars, including 8 planet-bearing stars, using the {\it Spitzer Space Telescope}. With accurate relative photometry using the Infrared…

We report the results of a spectroscopic search for debris disks surrounding 41 nearby solar type stars, including 8 planet-bearing stars, using the {\it Spitzer Space Telescope}. With accurate relative photometry using the Infrared…

We present an analysis of the dust attenuation of star forming galaxies at $z=2.5-4.0$ through the relationship between the UV spectral slope ($\beta$), stellar mass ($M_{\ast}$) and the infrared excess (IRX$=L_{\rm{IR}}/L_{\rm{UV}}$) based…

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