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JHK_S photometry is presented for a 35 arcmin square field centred on the Sculptor dwarf spheroidal galaxy. With the aid of published kinematic data definite galaxy members are identified and the width in J-K of the colour-magnitude diagram…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 John W. Menzies , Michael W. Feast , Patricia A. Whitelock , Noriyuki Matsunaga

We present deep CCD photometry of a field in the newly discovered dwarf spheroidal galaxy in Sagittarius (hereafter Sgr), and of a nearby control field. These data (totaling ~3.5 hrs exposure time in V and I) were used to produce…

Astrophysics · Physics 2009-10-22 Mario Mateo , A. Udalski , M. Szymanski , J. Kaluzny , M. Kubiak , W. Krzeminski

JHKs photometry is presented from a three-year survey of the central regions of the Local Group dwarf irregular galaxy IC1613. The morphologies of the colour-magnitude and colour-colour diagrams are discussed with particular reference to…

Astrophysics of Galaxies · Physics 2015-08-06 John W. Menzies , Patricia A. Whitelock , Michael W. Feast

We present spectroscopic observations from the {\it Spitzer Space Telescope} of six carbon-rich AGB stars in the Sagittarius Dwarf Spheroidal Galaxy (Sgr dSph) and two foreground Galactic carbon stars. The band strengths of the observed…

We conducted an optical monitoring survey of the Sagittarius dwarf irregular galaxy (SagDIG) during the period of June 2016 -- October 2017, using the 2.5-m Isaac Newton Telescope (INT) at La Palama. Our goal was to identify Long Period…

In a shallow near-infrared survey of the dwarf Irregular galaxy, NGC 3109, near the periphery of the Local Group, we have found eight Mira variables, seven of which appear to be oxygen-rich (O-Miras). The periods range from about 430 days…

Solar and Stellar Astrophysics · Physics 2018-12-26 J. W. Menzies , P. A. Whitelock , M. W. Feast , N. Matsunaga

Using multi-epoch JHK photometry obtained with the 1.4-m Japanese-South African Infrared Survey Facility at Sutherland we have identified large numbers of AGB variables in NGC 6822. This paper uses 30 large amplitude variables, with periods…

Astrophysics of Galaxies · Physics 2010-11-16 Francois Nsengiyumva , Patricia W. Whitelock , Michael W. Feast , John W. Menzies

We present deep BVRI CCD photometry of the stars in the dwarf irregular galaxy SagDIG. The color-magnitude diagrams of the measured stars in SagDIG show a blue plume which consists mostly of young stellar populations, and a well-defined red…

Astrophysics · Physics 2009-10-31 Myung Gyoon Lee , Sang Chul Kim

A study is made of a sample of 58 dust-enshrouded Asymptotic Giant Branch (AGB) stars (including 2 possible post AGB stars), of which 27 are carbon-rich and 31 are oxygen-rich. These objects were originally identified by Jura & Kleinmann as…

Astrophysics · Physics 2009-11-06 Enrico A. Olivier , Patricia Whitelock , Fred Marang

Using two HST/ACS data-sets that are separated by ~2 years has allowed us to derive the relative proper-motion for the Sagittarius dwarf irregular (SagDIG) and reduce the heavy foreground Galactic contamination. The proper-motion…

Astrophysics of Galaxies · Physics 2014-11-26 Y. Momany , M. Clemens , L. R. Bedin , M. Gullieuszik , E. V. Held , I. Saviane , S. Zaggia , L. Monaco , M. Montalto , R. M. Rich , L. Rizzi

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…

Solar and Stellar Astrophysics · Physics 2015-06-23 Megan Reiter , Massimo Marengo , Joseph L. Hora , Giovanni G. Fazio

The distance, star formation history and global properties of the Local Group dIrr galaxy SagDIG are derived based on an [I-(V-I)] colour--magnitude diagram of ~1550 stars. A distance of 1.06+/-0.10 Mpc is obtained from the I magnitude of…

Astrophysics · Physics 2007-05-23 I. Karachentsev , A. Aparicio , L. Makarova

Twenty six Asymptotic Giant Branch (AGB) variables are identified in the Local Group galaxy Leo I. These include 7 Mira and 5 semi-regular variables for which periods, amplitudes and mean magnitudes are determined. The large range of…

Astrophysics of Galaxies · Physics 2015-05-18 John W. Menzies , Patricia A. Whitelock , Michael W. Feast , Noriyuki Matsunaga

We present the results of a near-infrared monitoring programme of a selected sample of stars, initially suspected to be Mira variables and OH/IR stars, covering more than a decade of observations. The objects monitored cover the typical…

Astrophysics · Physics 2016-08-15 F. M. Jiménez-Esteban , P. García-Lario , D. Engels , A. Manchado

We present the third and final part of a census of Asymptotic Giant Branch (AGB) stars in Local Group dwarf irregular galaxies. Papers I and II presented the results for WLM and IC 1613. Included here are Phoenix, LGS 3, DDO 210, Leo A,…

Astrophysics of Galaxies · Physics 2011-02-11 Martha L. Boyer , Evan D. Skillman , Jacco Th. van Loon , Robert D. Gehrz , Charles E. Woodward

Low metallicity massive stars hold the key to interpret numerous processes in the past Universe including re-ionization, starburst galaxies, high-redshift supernovae and GRBs. The Sagittarius Dwarf Irregular Galaxy (SagDIG,…

Solar and Stellar Astrophysics · Physics 2017-12-01 Miriam Garcia

We present deep $BVI$ observations of the dwarf irregular galaxy UKS1927-177 in Sagittarius. Statistically cleaned $V$, $(B-I)$ CMDs clearly display the key evolutionary features in this galaxy. Previously detected C stars are located in…

Astrophysics · Physics 2009-11-07 Y. Momany , E. V. Held , I. Saviane , L. Rizzi

The main characteristics of a wide photometric survey of the Sgr dwarf spheroidal galaxy are shortly presented. V and I photometry has been obtained for ~ 90000 stars toward Sgr and for ~ 9000 stars in a region devoid of Sgr stars (for…

Astrophysics · Physics 2007-05-23 M. Bellazzini , F. R. Ferraro , R. Buonanno

Sagittarius (Sgr) is a massive disrupted dwarf spheroidal galaxy in the Milky Way halo that has undergone several stripping events. Previous chemical studies were restricted mainly to a few, metal- rich ([Fe/H]~ -1) stars that suggested a…

We have identified a new class of Asymptotic Giant Branch (AGB) stars in the Small and Large Magellanic Clouds (SMC/LMC) using optical to infrared photometry, light curves, and optical spectroscopy. The strong dust production and…

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