Results 131 to 140 of about 208,454 (264)
RR Lyrae binary systems in the Galactic bulge
The possibility of a direct mass measurement of RR Lyrae variable stars in binary systems has remained elusive for many years, due to the apparent paucity of such systems.
Hajdu Gergely, Catelan Márcio
doaj +1 more source
Are the Ogle Microlenses in the Galactic Bar?
The analysis of the first two years of OGLE data revealed 9 microlensing events of the galactic bulge stars, with the characteristic time scales in the range $ 8.6 < t_0 < 62 $ days, where $ t_0 = R_E / V $.
Kaluzny, J. +7 more
core +2 more sources
The inner Galactic bulge: evidence for a nuclear bar?
Recent data from the VVV survey have strengthened evidence for a structural change in the Galactic bulge inwards of |l|
Alves +17 more
core +1 more source
Bursty stellar populations and obscured active galactic nuclei in galaxy bulges [PDF]
Vivienne Wild +7 more
openalex +1 more source
A Breakdown of the Black Hole–Bulge Mass Relation in Local Active Galaxies
We investigate the relation between black hole (BH) mass and bulge stellar mass for a sample of 117 local ( z ∼ 0) galaxies hosting low-luminosity, broad-line active galactic nuclei (AGNs).
Megan R. Sturm, Amy E. Reines
doaj +1 more source
We present new UV-to-IR stellar photometry of four low-extinction windows in the Galactic bulge, obtained with the Wide Field Camera 3 on the Hubble Space Telescope (HST).
Anderson, Jay +16 more
core +1 more source
Theoretical Models of the Galactic Bulge [PDF]
Juntai Shen, Zhao‐Yu Li
openalex +1 more source
Tracing Back a Second-generation Star Stripped from Terzan 5 by the Galactic Bar
The Galactic bulge hosts the Milky Way’s oldest stars, possibly coming from disrupted globular clusters (GCs) or the bulge’s primordial building blocks, making these stars witnesses to the Galaxy’s early chemical enrichment.
Stefano O. Souza +8 more
doaj +1 more source
Two Red Clumps and the X-Shaped Milky Way Bulge
From 2MASS infra-red photometry we find two red clump (RC) populations co-existing in the same fields toward the Galactic bulge at latitudes |b|>5.5 deg., ranging over ~13 degrees in longitude and 20 degrees in latitude.
McWilliam, Andrew, Zoccali, Manuela
core +1 more source
Mass Distribution in Rotating Thin-Disk Galaxies According to Newtonian Dynamics
An accurate computational method is presented for determining the mass distribution in a mature spiral galaxy from a given rotation curve by applying Newtonian dynamics for an axisymmetrically rotating thin disk of finite size with or without a central ...
James Q. Feng, C. F. Gallo
doaj +1 more source

