Horizontal Branch Stars: The Interplay between Observations and Theory, and Insights into the Formation of the Galaxy
arXiv:astro-ph/0507464 · doi:10.1007/s10509-009-9987-8
Abstract
We review HB stars in a broad astrophysical context, including both variable and non-variable stars. A reassessment of the Oosterhoff dichotomy is presented, which provides unprecedented detail regarding its origin and systematics. We show that the Oosterhoff dichotomy and the distribution of globular clusters (GCs) in the HB morphology-metallicity plane both exclude, with high statistical significance, the possibility that the Galactic halo may have formed from the accretion of dwarf galaxies resembling present-day Milky Way satellites such as Fornax, Sagittarius, and the LMC. A rediscussion of the second-parameter problem is presented. A technique is proposed to estimate the HB types of extragalactic GCs on the basis of integrated far-UV photometry. The relationship between the absolute V magnitude of the HB at the RR Lyrae level and metallicity, as obtained on the basis of trigonometric parallax measurements for the star RR Lyrae, is also revisited, giving a distance modulus to the LMC of (m-M)_0 = 18.44+/-0.11. RR Lyrae period change rates are studied. Finally, the conductive opacities used in evolutionary calculations of low-mass stars are investigated. [ABRIDGED]
56 pages, 22 figures. Invited review, to appear in Astrophysics and Space Science
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- Core collapse and horizontal-branch morphology in galactic globular clusters
- Probing the Galactic halo with RR Lyrae stars -- IV. On the Oosterhoff dichotomy of RR Lyrae stars
- Evolution of the Ultraviolet Upturn at : exploring helium rich stellar populations
- Time-Series BVI Photometry for the Globular Cluster NGC 6981 (M72)
- Variable Stars in Large Magellanic Cloud Globular Clusters II: NGC 1786
- SMHASH: A new mid-infrared RR Lyrae distance determination for the Local Group dwarf spheroidal galaxy Sculptor
- Effect of Binary Fraction on Horizontal Branch Morphology under Tidally Enhanced Stellar Wind
- A new visit to the variable stars in M56 and its colour magnitude diagram structure
- The binary fraction of Blue Horizontal-Branch (BHB) Stars
- On the photometric metallicity of Oosterhoff-type I and II RRab stars
- Study of UV bright stellar populations in the globular cluster NGC 1261 using AstroSat
- Discovery of an extended Horizontal Branch in the Large Magellanic Cloud globular cluster NGC1835
- Where are the binaries? -- Searching for blue horizontal-branch stars in binary systems in the inner Galactic Halo
- The Power of Principled Bayesian Methods in the Study of Stellar Evolution
- Omega Centauri: weak MgH-band in red giants directly trace the helium content
- The Ultraviolet Upturn in field Luminous Red Galaxies at
- Diffuse LINER-type emission from extended disc regions of barred galaxies
- Period changes in the RR Lyrae stars of NGC 6171 (M107)
- Learning novel representations of variable sources from multi-modal data via autoencoders
- Study of UV bright sources in globular cluster NGC 4590 using Ultraviolet Imaging Telescope (UVIT) observations
- A fork in the Sagittarius trailing debris
- Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud: III. Horizontal Branch Morphology
- Variable stars in the VVV globular clusters. II. NGC6441, NGC6569, NGC6626 (M28), NGC6656 (M22), 2MASS-GC02, and Terzan10
- An Extreme Ultra-Compact X-ray Binary in a Globular Cluster: Multi-Wavelength Observations of RZ2109 Explored in a Triple System Framework
- Far Ultra-Violet Insights Into NGC 1399's Globular Cluster Population
- Reconsidering The Bailey Diagrams of ab-type RR Lyrae Stars, Metallicity-Mediated Evolution as the Direct Cause of the Oosterhoff Phenomenon
- Habitable Zones of Host Stars During the Post-MS Phase
- High-cadence stellar variability studies of RR Lyrae stars with DECam: New multi-band templates
- Extraction of Physical Parameters of RRab Variables using Neural Network based Interpolator
- The origin of B-type runaway stars based on kinematics
- RR Lyrae stars with variable mean magnitudes
- Connections between the cycle-to-cycle light curve and O-C variations of the Blazhko RR Lyrae stars
- Matching seismic masses for RR Lyrae-type and oscillating red horizontal-branch stars in M4
- WFPC2 UV survey of Galactic Globular Clusters. The Horizontal Branch temperature distribution
- Statistical analysis of Galactic globular cluster type properties
- Optical and near-infrared pulsation properties of RR Lyrae and Population II Cepheid variables in the Messier 15 globular cluster
- RR Lyrae stars in the newly discovered ultra-faint dwarf galaxy Centaurus I
- Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
- A Multiband Photometric Study of RR Lyrae Stars in M53 (NGC 5024)
- Old stellar systems in UV: resolved and integrated properties