Results 101 to 110 of about 2,386 (209)

Sample of LMXBs in the Galactic bulge - I. Optical and near-infrared constraints from the Virtual Observatory [PDF]

, 2010
Ivan Yu. Zolotukhin, Mikhail G. Revnivtsev   +1 more
openalex   +1 more source

LISA Galactic binaries in the Roman Galactic Bulge Time-Domain Survey

, 2023
Matthew C. Digman, Christopher M. Hirata
openalex   +2 more sources

Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]

Astron Astrophys Rev, 2023
Ruszkowski M, Pfrommer C.
europepmc   +1 more source

Microlensing Discovery and Characterization Efficiency in the Vera C. Rubin Legacy Survey of Space and Time

The Astrophysical Journal Supplement Series
The Vera C. Rubin Legacy Survey of Space and Time will discover thousands of microlensing events across the Milky Way, allowing for the study of populations of exoplanets, stars, and compact objects.
Natasha S. Abrams, Markus P. G. Hundertmark, Somayeh Khakpash, Rachel A. Street, R. Lynne Jones, Jessica R. Lu, Etienne Bachelet, Yiannis Tsapras, Marc Moniez, Tristan Blaineau, Rosanne Di Stefano, Martin Makler, Anibal Varela, Markus Rabus   +13 more
doaj   +1 more source

Shaping the relation between the mass of supermassive black holes and the velocity dispersion of galactic bulges [PDF]

, 2013
M. H. Chan
openalex   +1 more source

DRAFTS: A DEEP, RAPID ARCHIVAL FLARE TRANSIENT SEARCH IN THE GALACTIC BULGE [PDF]

, 2012
Rachel A. Osten, Adam Kowalski, Kailash Sahu, Suzanne L. Hawley   +3 more
openalex   +1 more source

Dynamical Origin of the Vertical Metallicity Gradient of the Milky Way Bulge

The Astrophysical Journal
A vertical metallicity gradient (VMG) in the Milky Way bulge is well-established. Yet, its origin has not been fully understood under the Galactic secular evolution scenario.
Bin-Hui Chen, Juntai Shen, Zhong Liu
doaj   +1 more source

Red-giant branch morphology of metal-poor globular clusters in the Galactic bulge [PDF]

, 2007
J. W. Kim, H. I. Kim, Young‐Jong Sohn
openalex   +1 more source

Formation Models of the Galactic Bulge

, 2014
The Galactic bulge is now considered to be the inner three-dimensional part of the Milky Way's bar. It has a peanut shape and is characterized by cylindrical rotation. In N-body simulations, box/peanut bulges arise from disks through bar and buckling instabilities.
openaire   +3 more sources

A massive quiescent galaxy at redshift 4.658. [PDF]

Nature, 2023
Carnall AC, McLure RJ, Dunlop JS, McLeod DJ, Wild V, Cullen F, Magee D, Begley R, Cimatti A, Donnan CT, Hamadouche ML, Jewell SM, Walker S.   +12 more
europepmc   +1 more source