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Related papers: A point source survey of M31 with the Spitzer Spac…

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We have carried out an infrared search for obscured AGB stars in the Magellanic Clouds. The survey uncovered a number of obscured AGB stars as well as some supergiants with infrared excess. We present photometry of the sources and discuss…

We have conducted a near-infrared monitoring campaign at the UK InfraRed Telescope (UKIRT), of the Local Group spiral galaxy M33 (Triangulum). The main aim was to identify stars in the very final stage of their evolution, and for which the…

Solar and Stellar Astrophysics · Physics 2015-05-27 Atefeh Javadi , Jacco Th. van Loon , Mohammad Taghi Mirtorabi

The binarity of red supergiants (RSGs) influences their evolution and the fate of supernovae. We investigate the binary fraction of RSGs in the Andromeda Galaxy (M31) and Triangulum Galaxy (M33) using photometry from the Hubble Space…

Solar and Stellar Astrophysics · Physics 2025-06-04 Min Dai , Shu Wang , Biwei Jiang , Ying Li

Studying the stellar populations in the outskirts of spiral galaxies can provide important constraints on their structure, formation, and evolution. To that end, we present VI photometry obtained with the Advanced Camera for Surveys for…

Astrophysics · Physics 2008-11-26 Michael K. Barker , Ata Sarajedini , Doug Geisler , Paul Harding , Robert Schommer

Wide-field JHKs near-infrared observations covering an area of 1.8x1.8 sq. deg. centred on M33 were obtained using WFCAM at UKIRT. These data show a large population of intermediate-age asymptotic giant branch stars (AGB). We have used both…

How does the submm galaxy population detected by SCUBA fit into galaxy evolution? How do these rare starbursting systems, which contribute significantly to high redshift star-formation, relate to other galaxy populations? Deep radio…

(Abridged) This work explores the existence of high redshift massive galaxies unveiled with Spitzer+IRAC, but missed by conventional selection techniques based on optical and near-infrared observations. To this end, we use the…

Astrophysics · Physics 2009-11-13 G. Rodighiero , A. Cimatti , A. Franceschini , M. Brusa , J. Fritz , M. Bolzonella

Asymptotic giant branch stars are essential contributors to the near and mid-IR emission of intermediate age (0.1-1Gyr old) stellar populations. Detecting this light sets constraints on the star formation history in galaxies and,…

Astrophysics · Physics 2007-05-23 A. Lancon

We examine the nature of the progenitor of the giant stellar stream in M31 using as constraints new radial velocity measurements of stream red giant stars (presented in the companion paper by Guhathakurta et al. 2005, astro-ph/0406145)…

We explore the effects of stellar population models on estimating star formation histories, ages and masses of high redshift galaxies. The focus is on the Thermally-Pulsing Asymptotic Giant Branch (TP-AGB) phase of stellar evolution, whose…

Astrophysics · Physics 2008-11-26 C. Maraston , E. Daddi , A. Renzini , A. Cimatti , M. Dickinson , C. Papovich , A. Pasquali , N. Pirzkal

We present new modelling of the spectrophotometric properties of intermediate age stellar populations in the near-infrared (NIR). We take into account the evolutionary and spectroscopic properties of the Asymptotic Giant Branch (AGB) stars…

Astrophysics · Physics 2007-05-23 M. Mouhcine , A. Lancon

Images obtained with NIRI on the Gemini North telescope are used to investigate the photometric properties of the central regions of M31 in the 3 - 5 micron wavelength range. The light distribution in the central arcsecond differs from what…

Astrophysics · Physics 2008-11-26 T. J. Davidge , Joseph B. Jensen , K. A. G. Olsen

Observing objects in transition from pre- to young Planetary Nebula (PN), when the central star radiation starts to excite the envelope, can help us to understand the evolution of the circumstellar ejecta and their shaping mechanism/s. In…

Astrophysics · Physics 2007-09-03 L. Cerrigone , J. L. Hora , G. Umana , C. Trigilio

High-redshift submillimetre-bright galaxies identified by blank field surveys at millimetre and submillimetre wavelengths appear in the region of the IRAC colour-colour diagrams previously identified as the domain of luminous active…

The Spitzer Space Telescope revolutionized studies of Active Galactic Nuclei (AGNs). Its combined sensitivity and mapping speed at mid-infrared wavelengths revealed a substantial population of highly-obscured AGNs. This population implies a…

Astrophysics of Galaxies · Physics 2020-08-13 Mark Lacy , Anna Sajina

We present the sample for an abundance analysis of 25 members of M71 with luminosities ranging from the red giant branch tip to the upper main sequence. The spectra are of high dispersion and of high precision. We describe the observing…

Astrophysics · Physics 2009-11-06 Judith G. Cohen , Bradford B. Behr , Michael M. Briley

Yellow and red supergiants are evolved massive stars whose numbers and locations on the HR diagram can provide a stringent test for models of massive star evolution. Previous studies have found large discrepancies between the relative…

Solar and Stellar Astrophysics · Physics 2015-06-04 Maria R. Drout , Philip Massey , Georges Meynet

We present Faint Object Camera (FOC) ultraviolet images of the central 14x14'' of Messier 31 and Messier 32. The hot stellar population detected in the composite UV spectra of these nearby galaxies is partially resolved into individual…

Astrophysics · Physics 2009-10-30 T. M. Brown , H. C. Ferguson , S. A. Stanford , J. -M. Deharveng

We present Spitzer high spectral resolution IRS spectroscopy of three positions in the carbon-rich outflow of post-AGB star HD 44179, better known as the Red Rectangle. Surprisingly, the spectra show some strong unknown mid-infrared…

Astrophysics · Physics 2009-11-13 F. Markwick-Kemper , J. D. Green , E. Peeters

We summarize observations with the Spitzer Infrared Spectrograph (IRS) of 571 starbursts (strong PAH emission features), 128 obscured AGN (strong silicate absorption), and 39 unobscured AGN (silicate emission). Sources range in luminosity…

Cosmology and Nongalactic Astrophysics · Physics 2010-05-04 James R. Houck , Daniel W. Weedman
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