Results 81 to 90 of about 47,309 (203)

Attenuation modified by DIG and dust as seen in M31

open access: yes, 2017
The spatial distribution of dust in galaxies affects the global attenuation, and hence inferred properties, of galaxies. We trace the spatial distribution of dust in five fields (at 0.6-0.9 kpc scale) of M31 by comparing optical attenuation with the ...
Blanc, Guillermo A.   +7 more
core   +1 more source

First microlensing candidate towards M31 from the Nainital Microlensing Survey [PDF]

open access: yes, 2004
We report our first microlensing candidate NMS-E1 towards M31 from the data accumulated during the four years of Nainital Microlensing Survey. Cousin R and I band observations of ~13'x13' field in the direction of M31 have been carried out since 1998 and
A. K. Pandey   +31 more
core   +2 more sources

Predicative Possession in Ukrainian and Intra‐Slavonic Language Contact1

open access: yesTransactions of the Philological Society, Volume 123, Issue 3, Page 428-459, November 2025.
Abstract Ukrainian has two inherited syntactic forms for possessive have: a transitive one with a lexical have‐verb, and an intransitive, originally locative be‐construction. On the basis of four corpus studies, the article establishes their relative frequency in Middle Ukrainian writing (17th and 18th c.), Modern Ukrainian dialects (20th c.), and ...
Jan Fellerer
wiley   +1 more source

Properties of M31. II: A Cepheid disk sample derived from the first year of PS1 PAndromeda data

open access: yes, 2013
We present a sample of Cepheid variable stars towards M31 based on the first year of regular M31 observations of the PS1 survey in the r_P1 and i_P1 filters.
Bender, Ralf   +16 more
core   +1 more source

A Comprehensive Catalog of Emission-line Nebulae, Star Clusters, and Supergiants in M31 from the LAMOST Spectroscopic Survey

open access: yesThe Astronomical Journal
Spectroscopic observations of various tracers in nearby galaxies, such as Andromeda (M31), play a crucial role in identifying and classifying individual stellar populations and nebular objects, thereby enhancing our understanding of galactic composition,
Pinjian Chen   +7 more
doaj   +1 more source

Supersoft X-ray sources in M31 [PDF]

open access: yes, 2007
8 pages postscript incl. figures, Proc. of Workshop on Supersoft X-Ray Sources, to appear in Lecture Notes in Physics vol. 472 (1996)
Greiner, J., Supper, R., Magnier, E. A.
openaire   +2 more sources

Theory of pixel lensing towards M31 I: the density contribution and mass of MACHOs

open access: yes, 2000
POINT-AGAPE is an Anglo-French collaboration which is employing the Isaac Newton Telescope (INT) to conduct a pixel-lensing survey towards M31. In this paper we investigate what we can learn from pixel-lensing observables about the MACHO mass and ...
Carr, B. J.   +8 more
core   +2 more sources

Efficacy and field safety of ilunocitinib for the control of atopic dermatitis in client‐owned dogs: A multicentre, double‐masked, randomised, placebo‐controlled clinical trial

open access: yesVeterinary Dermatology, Volume 36, Issue 5, Page 647-659, October 2025.
Background – Inhibition of the Janus kinase (JAK) pathway is a well‐established option for canine atopic dermatitis (cAD). Objective – To evaluate the efficacy and safety of ilunocitinib, a novel JAK inhibitor for the control of pruritus and skin lesions in client‐owned dogs with cAD.
Sophie Forster   +5 more
wiley   +1 more source

Fifteen Years of M31* X-Ray Variability and Flares

open access: yesThe Astrophysical Journal
We append an additional 15 yr (2009–2024) to the Chandra X-ray light curve of M31*, the supermassive black hole (SMBH) at the center of M31, the Andromeda galaxy. Extending and expanding on the work in Z.
Stephen DiKerby, Shuo Zhang, Jimmy Irwin
doaj   +1 more source

The Bulge of M31 [PDF]

open access: yesPublications of the Astronomical Society of Australia, 2013
AbstractBulges are not just elliptical subgalaxies situated in the centers of large spirals, though it might seem so from their ages and chemistry. In fact, bulge kinematics have been known to be different since the first long slit spectra were obtained.
openaire   +3 more sources

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