Results 11 to 20 of about 51,668 (266)
The reported positions of 964 suspected nova eruptions in M31 recorded through the end of calendar year 2013 have been compared in order to identify recurrent nova candidates. To pass the initial screen and qualify as a recurrent nova candidate two or more eruptions were required to be coincident within 0.1', although this criterion was relaxed to 0.15'
Shafter, A. W. +10 more
openaire +7 more sources
Abstract We have analysed Herschel observations of M31, using the ppmap procedure. The resolution of ppmap images is sufficient ($\sim 31\, {\rm pc}$ on M31) that we can analyse far-IR dust emission on the scale of giant molecular clouds.
A P Whitworth +8 more
openaire +4 more sources
Close inspection of the channel maps which make up the high resolution M31 HI-data set (Brinks, this volume) resulted in finding numerous shell structures and bubble-like regions. To avoid any bias in the interpretation we shall call holes, in the course of this contribution, all those structures where we find a deficiency of neutral gas.
E. Brinks, E. Bajaja
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The authors wish to make the following corrections to this paper [...]
Alistair J. McBurnie +3 more
doaj +1 more source
Newly Discovered Wolf–Rayet Stars in M31
The evolved massive star populations of the Local Group galaxies are generally thought to be well understood. However, recent work has suggested that the Wolf–Rayet (WR) content of M31 may have been underestimated.
Kathryn F. Neugent, Philip Massey
doaj +1 more source
Planetary Nebula Kinematics in M31 [PDF]
accepted to ApJ; main body of paper is 36 pages, including 14 ...
Hurley-Keller, Denise +3 more
openaire +2 more sources
M31* and its circumnuclear environment [PDF]
Submitted to MNRAS, 33 pages, 9 figures.
Li, Z, Wang, QD, Wakker, BP
openaire +3 more sources
Microlensing towards LMC and M31 [PDF]
The nature and the location of the lenses discovered in the microlensing surveys done so far towards the LMC remain unclear. Motivated by these questions we computed the optical depth for the different intervening populations and the number of expected events for self-lensing, using a recently drawn coherent picture of the geometrical structure and ...
jetzer, Ph. +2 more
openaire +4 more sources
The Chemodynamics of the Stellar Populations in M31 from APOGEE Integrated-light Spectroscopy
We present an analysis of nearly 1000 near-infrared, integrated-light spectra from APOGEE in the inner ∼7 kpc of M31. We utilize full-spectrum fitting with A-LIST simple stellar population spectral templates that represent a population of stars with the ...
Benjamin J. Gibson +10 more
doaj +1 more source
This study aimed to examine the effects of change of direction (COD) speed and technique modification training on 180° turning performance (completion time, ground contact time [GCT], and exit velocity), kinetics, and kinematics.
Thomas Dos’Santos +4 more
doaj +1 more source

