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Related papers: Spitzer/IRAC Observations of AGB stars

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Spitzer/IRAC color selection is a promising technique to identify hot accreting nuclei, that is to say AGN, in galaxies. We demonstrate this using a small sample of SAURON galaxies, and explore this further. The goal of this study is to…

Astrophysics of Galaxies · Physics 2020-08-19 Tuba İkiz , Reynier F. Peletier , Peter D. Barthel , Cahit Yeşilyaprak

In this work, a sample of luminous M-type giants in the Baade's Windows towards the inner Galactic Bulge is investigated in the near-infrared. The ISOGAL survey at 7 and 15 micron has given information concerning the mass-loss rates of…

Astrophysics · Physics 2007-05-23 M. Schultheis , I. S. Glass

While the importance of dusty asymptotic giant branch (AGB) stars to galactic chemical enrichment is widely recognised, a sophisticated understanding of the dust formation and wind-driving mechanisms has proven elusive due in part to the…

Solar and Stellar Astrophysics · Physics 2015-06-11 T. D. Blasius , J. D. Monnier , P. G. Tuthill , W. C. Danchi , M. Anderson

We present the first mid-infrared spectra of SMP LMC 11 in the Large Magellanic Cloud. While this object resembles a planetary nebula in the optical, its infrared properties are more similar to an object in transition from the asymptotic…

Astrophysics · Physics 2009-11-11 J. Bernard-Salas , E. Peeters , G. C. Sloan , J. Cami , S. Guiles , J. R. Houck

We report Spitzer Space Telescope photometry of eleven externally-polluted white dwarfs. Of the nine stars for which we have IRAC photometry, we find that GD 40, GD 133 and PG 1015+161 each has an infrared excess that can be understood as…

Astrophysics · Physics 2009-06-23 M. Jura , J. Farihi , B. Zuckerman

We analyze very deep HST, VLT and Spitzer photometry of galaxies at 2<z<3.5 in the Hubble Deep Field South. The sample is selected from the deepest public K-band imaging currently available. We show that the rest-frame U-V vs V-J…

We present high resolution optical spectroscopic observations of IRAS 09425-6040, a peculiar, extremely red, C-rich AGB star showing prominent O-rich dust features in its ISO infrared spectrum attributed to crystalline silicates. Our…

Astrophysics · Physics 2009-11-11 D. A. Garcia-Hernandez , C. Abia , A. Manchado , P. Garcia-Lario

We aim to constrain the dust mass and grain sizes in the interaction regions between the stellar winds and the ISM around asymptotic giant branch stars. By describing the dust in these regions, we aim to shed light on the role of low mass…

Astrophysics of Galaxies · Physics 2022-09-21 M. Maercker , T. Khouri , M. Mecina , E. De Beck

We present a mid-infrared (IR) sample study of nearby ultraluminous X-ray sources (ULXs) using multi-epoch observations with the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. Spitzer/IRAC observations taken after 2014 were…

We present 20 band photometry from the far-IR to X-ray in the Spitzer IRAC dark field. The bias for the near-IR camera on Spitzer is calibrated by observing a ~20 arcminute diameter "dark" field near the north ecliptic pole roughly every…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 J. E. Krick , J. A. Surace , D. Thompson , M. L. N. Ashby , J. Hora , V. Gorjian , L. Yan , D. T. Frayer , E. Egami , M. Lacy

It is still an unresolved problem how much AGB stars can contribute to the overall gas and dust enrichment processes in the interstellar medium within galaxies. We start tackling this problem, by using our test case observational data from…

Cosmology and Nongalactic Astrophysics · Physics 2010-11-09 M. Matsuura

We surveyed 20 AGB stars of different chemical types using the APEX telescope, and combined this with an IRAM 30 m and APEX survey of CS and SiS emission towards over 30 S-type stars. For those stars with detections, we performed radiative…

Solar and Stellar Astrophysics · Physics 2018-10-03 T. Danilovich , S. Ramstedt , D. Gobrecht , L. Decin , E. De Beck , H. Olofsson

Benefiting from the GAIA second and early third releases of photometric and astrometric data we examine the population of asymptotic giant branch (AGB) stars that appear in the fields of intermediate-age and young open star clusters. We…

We have searched for near-infrared stellar counterparts of IRAS point sources in the Large Magellanic Cloud (LMC), in J and K-bands. This resulted in the detection of 21 counterparts, of which 19 are new discoveries. Using colour-magnitude…

Photometric maps, obtained with Spitzer's Infrared Array Camera (IRAC), can provide a valuable probe of warm molecular hydrogen within the interstellar medium. IRAC maps of the supernova remnant IC443, extracted from the Spitzer archive,…

Astrophysics · Physics 2009-11-13 David Neufeld , Yuan Yuan

Diffuse interstellar bands comprise hundreds of absorption features in the ISM. Most DIBs are observed in the optical, but some are in the IR. We observed 76 early-type stars at R=50,000 and S/N ratios of several hundreds using CRIRES. We…

We present mid-infrared to optical properties of 22 representative irregular galaxies: 18 Im, 3 BCDs, and one Sm. The mid-IR is based on images from the Spitzer Space Telescope archives. The 3.6 and 4.5 micron bands and the UBVJHK images…

Astrophysics · Physics 2008-11-26 Deidre A. Hunter , Bruce G. Elmegreen , Emily Martin

We present spectroscopic results for all galaxies observed with the Spitzer Infrared Spectrograph (IRS) which also have total infrared fluxes f(ir) measured with the Infrared Astronomical Satellite (IRAS), also using AKARI photometry when…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-08 Lusine Sargsyan , Daniel Weedman , Vianney Lebouteiller , James Houck , Donald Barry , Ashot Hovhannisyan , Areg Mickaelian

We present measurements of the 3.4-micron hydrocarbon dust absorption feature, and four visual diffuse interstellar bands, for twelve highly reddened (9.0<A(V)<15.8), early-type stars identified from the Stephenson (1992) catalogue,…

Astrophysics · Physics 2009-11-07 M. G. Rawlings , A. J. Adamson , D. C. B. Whittet

We present 43 GHz VLA spectra for 51 AGB sources with the goal of verifying an infrared (IR) color cut intended to separate Carbon-rich (C) and Oxygen-rich (O) AGB sources throughout the Galaxy. The color cut is a simple line in the…

Solar and Stellar Astrophysics · Physics 2020-10-07 Megan O. Lewis , Ylva M. Pihlström , Loránt O. Sjouwerman , Luis Henry Quiroga-Nuñez
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