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Related papers: An evolutionary catalogue of Galactic post-AGB and…

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Local Group (LG) very metal-poor massive stars are the best proxy for the First Stars of the Universe and fundamental to modelling the evolution of early galaxies. These stars may follow new evolutionary pathways restricted to very low…

Astrophysics of Galaxies · Physics 2022-08-03 Marta Lorenzo , Miriam Garcia , Francisco Najarro , Artemio Herrero , Miguel Cerviño , Norberto Castro

A significant number of the parameters of a gamma-ray burst (GRB) and its host galaxy are calculated from the afterglow. There are various methods obtaining extinction values for the necessary correction for galactic foreground. These are:…

In order to determine the composition of the dust in the circumstellar envelopes of oxygen-rich asymptotic giant branch (AGB) stars we have computed a grid of modust radiative-transfer models for a range of dust compositions, mass-loss…

Solar and Stellar Astrophysics · Physics 2015-06-18 O. C. Jones , F. Kemper , S. Srinivasan , I. McDonald , G. C. Sloan , A. A. Zijlstra

This paper describes the identification of Gaia counterparts of a sample of oxygen-rich AGB stars with OH maser emission as a first step towards the compilation of a general Gaia Catalogue of Galactic AGB stars. With this catalogue, tests…

Solar and Stellar Astrophysics · Physics 2025-06-04 Belén López Martí , Francisco M. Jiménez Esteban , Dieter Engels , Pedro García Lario

Extended and updated grids of TP-AGB tracks have been implemented in the TRILEGAL population synthesis code, which generates mock stellar catalogues for a galaxy given its mass, distance, star formation history and age-metallicity relation,…

Astrophysics · Physics 2007-05-23 Leo Girardi , Paola Marigo

We present results of an all-sky hard X-ray survey based on almost four years of observations with the IBIS telescope on board the INTEGRAL observatory. The dead time-corrected exposure of the survey is ~33 Ms. Approximately 12% and 80% of…

Astrophysics · Physics 2009-11-13 R. Krivonos , M. Revnivtsev , A. Lutovinov , S. Sazonov , E. Churazov , R. Sunyaev

We present a catalogue of 233 BL Lacertae objects compiled through an extensive bibliographic search updated to mid-1995. A large fraction of the sources listed in the catalogue belongs to well-defined samples and can be used for…

Astrophysics · Physics 2015-06-24 Paolo Padovani , Paolo Giommi

We present a new catalogue of high mass X-ray binaries (HMXBs) in the Galaxy that we call the Galactic High Mass X-ray Binary Catalogue (XRBcats), which improves upon the most recent of such catalogues. We include new HMXBs discovered since…

High Energy Astrophysical Phenomena · Physics 2023-09-25 Marvin Neumann , Artur Avakyan , Victor Doroshenko , Andrea Santangelo

We present observations of 86 post-Asymptotic Giant Branch (post-AGB) stars of OH maser transitions, taken with the Parkes Telescope between September 2002 and August 2003. Post-AGB stars are the precursors of planetary nebulae, which have…

Astrophysics · Physics 2007-05-23 R. M. Deacon , A. J. Green , J. M. Chapman

Identifying Active Galactic Nuclei (AGNs) through their X-ray emission is efficient, but necessarily biased against X-ray-faint objects. We aim to characterize this bias by comparing X-ray-selected AGNs to the ones identified through…

The post-asymptotic giant branch (AGB) phase is arguably one of the least understood phases of the evolution of low- and intermediate- mass stars. The recent post-AGB evolutionary sequences computed by Miller Bertolami (2016) are at least…

Solar and Stellar Astrophysics · Physics 2017-11-29 Marcelo M. Miller Bertolami

Globular clusters are large collections of old stars that are orbiting the core of a galaxy. Our Milky Way Galaxy has about 160 known clusters, with perhaps more to be discovered. We first accumulated the necessary parameters for 16…

High Energy Astrophysical Phenomena · Physics 2017-12-22 Hambeleleni Ndiyavala , Christo Venter , Petrus Paulus Kruger

We investigate infrared properties of OGLE4 Mira variables in our Galaxy. For each object, we cross-identify the AllWISE, 2MASS, Gaia, and IRAS counterparts. We present various IR two-color diagrams (2CDs) and period-magnitude and…

Solar and Stellar Astrophysics · Physics 2023-01-11 Kyung-Won Suh

This paper is part of a larger project in which we systematically study the chemical abundances of Galactic and extragalactic post-asymptotic giant branch (post-AGB) stars. Lead (Pb) is the final product of the s-process nucleosynthesis and…

Solar and Stellar Astrophysics · Physics 2016-02-17 Kenneth De Smedt , Hans Van Winckel , Devika Kamath , Lionel Siess , Stephane Goriely , Amanda I. Karakas , Rajeev Manick

FUSE spectroscopy has proved that extremely hot hydrogen-deficient post-AGB stars (PG1159 stars) display matter on their surface that usually remains hidden in the region between the H- and He-burning shells of the former AGB star. Hence,…

Astrophysics · Physics 2007-05-23 K. Werner , T. Rauch , J. W. Kruk

We present a library of 139 near-IR spectra of cool asymptotic giant branch stars that will be useful for comparison with theoretical model atmosphere calculations and for modeling the integrated emission from intermediate-age stellar…

Solar and Stellar Astrophysics · Physics 2015-05-14 N. J. Wright , M. J. Barlow , R. Greimel , J. E. Drew , M. Matsuura , Y. C. Unruh , A. A. Zijlstra

We present X-ray data for a complete sample of 44 luminous infrared galaxies (LIRGs), obtained with the Chandra X-ray Observatory. These are the X-ray observations of the high luminosity portion of the Great Observatory All-sky LIRG Survey…

Data are given for 16 extragalactic objects (predominantly AGN) behind the Magellanic Clouds and for 146 quasar candidates behind the nearby galaxies NGC 45, 185, 253, 2366, 2403 and 6822, IC 1613, M31 and M33. The Magellanic Cloud objects…

Astrophysics · Physics 2009-10-30 David Crampton , G. Gussie , A. P. Cowley , P. C. Schmidtke

We present a systematic study of gamma-ray blazar candidates based on a sample of 40 objects taken from the WIBR catalogue. By using a likelihood analysis, 26 of the 40 sources showed significant gamma-ray signatures $\geq3\sigma$. Using…

High Energy Astrophysical Phenomena · Physics 2021-07-14 Blessing Musiimenta , Bruno Sversut Arsioli , Edward Jurua , Tom Mutabazi