OGLE small amplitude red giant variables in the Galactic Bar
arXiv:astro-ph/0310578 · doi:10.1111/j.1365-2966.2004.07587.x
Abstract
Among over 200,000 Galactic Bulge variable stars in the public domain OGLE catalogue, we found over 15,000 red giant variables following two well defined period -- amplitude relations. The periods are in the range 10 < P < 100 days, and amplitudes in the range 0.005 < A < 0.13 mag in I-band. The variables cover a broad range of reddening corrected colours, 1 < (V-I)_0 < 5, and a fairly narrow range of extinction corrected apparent magnitudes, 10.5 < I_0 < 13 . A subset of variables (type A) has a rms scatter of only 0.44 mag. The average magnitudes for these stars are well correlated with the Galactic longitude, and vary from I_{k,0} = 11.82 for l = +8 deg to I_{k,0} = 12.07 for l = -5 deg, clearly indicating that they are located in the Galactic Bar. Most variables have several oscillation periods.
15 pages, 9 figures (7 in low resolution), submitted to MNRAS. Article in full resolution can be obtained at http://www.astro.princeton.edu/~leyer/wrayetal.ps
References in corpus (9)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Modelling the Galactic Bar Using Red Clump Giants
- Color-Magnitude Diagram Distribution of the Bulge Red Clump Stars - Evidence for the Galactic Bar
- Variable Stars in the Magellanic Clouds: Results from OGLE and SIRIUS
- Oscillations of alpha UMa and other red giants
- Red variables in the OGLE-II database. I. Pulsations and period-luminosity relations below the tip of the Red Giant Branch of the LMC
- Long Period Variables detected by ISO in the SMC
- Solar-like oscillations of semiregular variables
- Period-magnitude relations for M giants in Baade's Window NGC6522
Cited by in corpus (50)
- No large population of unbound or wide-orbit Jupiter-mass planets
- Chemical tagging with APOGEE: Discovery of a large population of N-rich stars in the inner Galaxy
- Period-luminosity relations in evolved red giants explained by solar-like oscillations
- Gaia Data Release 2: The first Gaia catalogue of long-period variable candidates
- Gaia Data Release 3: The second Gaia catalogue of Long-Period Variable candidates
- Mira Variables in the OGLE Bulge fields
- Variable stars in the Magellanic Clouds: II. The data and infrared properties
- Variable stars across the observational HR diagram
- Near-Infrared Photometry of Globular Clusters Towards the Galactic Bulge: Observations and Photometric Metallicity Indicators
- Two new free-floating or wide-orbit planets from microlensing
- Active Learning to Overcome Sample Selection Bias: Application to Photometric Variable Star Classification
- Modelling Long-Period Variables - I. A new grid of O-rich and C-rich pulsation models
- Automated classification of variable stars for ASAS 1-2 data
- Non-adiabatic Oscillations of Red Giants
- Period-luminosity relations of pulsating M giants in the solar neighbourhood and the Magellanic Clouds
- MOA-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf Boundary
- Red variables in the OGLE-II data base -- III. Constraints on the three-dimensional structures of the LMC and SMC
- Mira variables in the Galactic bulge with OGLE-II data
- Pulsation Modes of Long-Period Variables in the Period-Luminosity Plane
- The ASAS-SN Catalog of Variable Stars IV: Periodic Variables in the APOGEE Survey
- Long-term photometry and periods for 261 nearby pulsating M giants
- Gaia Data Release 3: Microlensing Events from All Over the Sky
- MKT J170456.2-482100: the first transient discovered by MeerKAT
- Limits on planetary-mass primordial black holes from the OGLE high-cadence survey of the Magellanic Clouds
- The Wendelstein Calar Alto Pixellensing Project (WeCAPP): The M31 Variable Star Catalogue
- Long Period Variables in the Large Magellanic Cloud from the EROS-2 survey
- Semiregular variables with periods lying between the period-luminosity sequences C', C and D
- Acoustic oscillations in stars near the tip of the red giant branch
- Variable stars in the dwarf irregular galaxy NGC 6822: the photometric catalogue
- Period-luminosity diagram of long period variables in the Magellanic Clouds. New aspects revealed from Gaia Data Release 2
- Standard candles from the Gaia perspective
- Late-type giant variables in NGC6522, LMC and SMC: How do they differ?
- XMM observation of 1RXS J180431.1-273932: a new M-type X-ray binary with a 494 s-pulse period neutron star?
- Semi-regular red giants as distance indicators I. The period-luminosity relations of semi-regular variables revisited
- New type II Cepheids from VVV data towards the Galactic center
- Optical identification of X-ray source 1RXS J180431.1-273932 as a magnetic cataclysmic variable
- The OGLE Collection of Variable Stars. One Thousand Heartbeat Stars in the Galactic Bulge and Magellanic Clouds
- Variable classification in the LSST era: Exploring a model for quasi-periodic light curves
- Turbulent convection and pulsation stability of stars - III. Non-adiabatic oscillations of red giants
- The variability behavior of CoRoT M-giant Stars
- Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars
- Long-term Stellar Variability in the Galactic Centre Region
- Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE - Constellation
- The TAOS Project Stellar Variability II. Detection of 15 Variable Stars
- Detecting long-period variability in SDSS Stripe 82 standards catalog
- Calibrating and standardizing the Tip of the Red Giant Branch in the Small Magellanic Cloud using small-amplitude red giants
- The red giant branch tip in the SDSS, PS1, JWST, NGRST and Euclid photometric systems. Calibration in optical passbands using Gaia DR3 synthetic photometry
- Tracking Advanced Planetary Systems (TAPAS) with HARPS-N VII. Elder suns with low-mass companions
- MOA-2019-BLG-008Lb: a new microlensing detection of an object at the planet/brown dwarf boundary
- Understanding the Galaxy