Results 91 to 100 of about 7,749 (214)

Project AMIGA: The Inner Circumgalactic Medium of Andromeda from Thick Disk to Halo

open access: yesThe Astrophysical Journal
The inner circumgalactic medium (CGM) of galaxies, where disk and halo processes intersect, remains poorly characterized despite its critical role in regulating galaxy evolution.
Nicolas Lehner   +24 more
doaj   +1 more source

A survey of eclipsing binary stars in the eastern spiral arm of M31 [PDF]

open access: bronze, 2005
I. Todd   +5 more
openalex   +1 more source

The Molecular Clouds of M31

open access: yesThe Astrophysical Journal
Deep interferometric observations of CO and dust continuum emission are obtained with the Submillimeter Array at 230 GHz to investigate the physical nature of the giant molecular cloud (GMC) population in the Andromeda galaxy (M31).
Charles J. Lada   +3 more
doaj   +1 more source

A Kinematically Selected, Metal‐poor Stellar Halo in the Outskirts of M31 [PDF]

open access: bronze, 2006
S. C. Chapman   +6 more
openalex   +1 more source

A Short-Timescale Candidate Microlensing Event in the POINT-AGAPE Pixel Lensing Survey of M31 [PDF]

open access: bronze, 2001
M. Aurière   +16 more
openalex   +1 more source

The Role of Pressure in the Structure and Stability of GMCs in the Andromeda Galaxy

open access: yesThe Astrophysical Journal
We revisit the role of pressure in the structure, stability, and confinement of Giant Molecular Clouds (GMCs) in light of recently published observations and analysis of the GMCs in the Andromeda galaxy (M31). That analysis showed that, in the absence of
Charles J. Lada   +3 more
doaj   +1 more source

Classical novae from the POINT–AGAPE microlensing survey of M31 – II. Rate and statistical characteristics of the nova population [PDF]

open access: bronze, 2006
M. J. Darnley   +19 more
openalex   +1 more source

Bar-driven Gas Dynamics of M31

open access: yesThe Astrophysical Journal
The large-scale gaseous shocks in the bulge of M31 can be naturally explained by a rotating stellar bar. We use gas dynamical models to provide an independent measurement of the bar pattern speed in M31.
Zi-Xuan Feng   +7 more
doaj   +1 more source

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