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相关论文: The Tip of the Red Giant Branch

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New empirical calibrations of the Red Giant Branch Tip in the I,J,H and K bands based on two fundamental pillars, namely omega Centauri and 47 Tucanae, have been obtained by using a large optical and near infrared photometric database. Our…

天体物理学 · 物理学 2009-11-10 M. Bellazzini , F. R. Ferraro , A. Sollima , E. Pancino , L. Origlia

We present the ultimate I-band calibration of the tip of the red giant branch (TRGB) standard candle. Our calibration is based on photometry from the outer parts of the Large Magellanic Cloud, 2.75<r<6.5 degs from the center, collected…

The tip of the red giant branch (TRGB) is a well-established standard candle used to measure distances to nearby galaxies. The TRGB luminosity is typically measured in the I-band, where the luminosity has little dependency on stellar age or…

星系天体物理 · 物理学 2019-07-31 Kristen. B. W. McQuinn , Martha Boyer , Evan D. Skillman , Andrew E. Dolphin

The Tip of the Red Giant Branch provides a luminous standard candle for calibrating distance ladders that reach Type Ia supernova (SN Ia) hosts. However, recent work reveals that tip measurements vary at the $\sim$ 0.1 mag level for…

We present new empirical calibrations of the Red Giant Branch (RGB) Bump and Tip based on a homogeneous near-Infrared database of 24 Galactic Globular Clusters. The luminosities of the RGB Bump and Tip in the J, H and K bands and their…

天体物理学 · 物理学 2009-11-10 E. Valenti , F. R. Ferraro , L. Origlia

We use synthetic photometry from Gaia DR3 BP and RP spectra for a large selected sample of stars in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) to derive the magnitude of the Red Giant Branch (RGB) tip for these two…

星系天体物理 · 物理学 2024-11-06 M. Bellazzini , R. Pascale

We have obtained an accurate estimate of the absolute I magnitude of the Tip of the Red Giant Branch (M_I(TRGB)) for the globular cluster Omega Cen, based {\em (a)} on the largest photometric database ever assembled for a globular, by…

天体物理学 · 物理学 2007-05-23 Michele Bellazzini , Francesco R. Ferraro , Elena Pancino

The brightness of the tip of the Red Giant Branch is a useful reference quantity for several fields of astrophysics. An accurate theoretical prediction is needed for such purposes. Aims. We intend to provide a solid theoretical prediction…

太阳与恒星天体物理 · 物理学 2017-10-04 Aldo Serenelli , Achim Weiss , Santi Cassisi , Maurizio Salaris , Adriano Pietrinferni

Indications from Gaia data release 2 (DR2) are that the tip of the red giant branch (TRGB, a population II standard candle related to the helium flash in low mass stars) is close to -4 in absolute I magnitude in the Cousins photometric…

星系天体物理 · 物理学 2019-02-20 Jeremy Mould , Gisella Clementini , Gary Da Costa

We introduce a modified detection method for measuring the luminosity of the tip of the red giant branch (TRGB) by introducing the composite magnitude T = I - beta [(V-I)_o - 1.50], where beta is the slope of the tip magnitude as a function…

天体物理学 · 物理学 2008-12-18 Barry F. Madore , Violet Mager , Wendy L. Freedman

The tip of the red giant branch (TRGB) is an important standard candle for determining luminosity distances. Although several $10^5$ small amplitude red giant stars (SARGs) have been discovered, variability was previously considered…

宇宙学与河外天体物理 · 物理学 2024-03-05 Richard I. Anderson , Nolan W. Koblischke , Laurent Eyer

We have detected the tip of the Red Giant Branch (TRGB) in the solar neighborhood using near infrared photometry from the 2MASS and DIRBE catalogs, and revised Hipparcos parallaxes. We confirm that the revised Hipparcos parallaxes are…

太阳与恒星天体物理 · 物理学 2015-05-14 Vello Tabur , Laszlo L. Kiss , Timothy R. Bedding

We present a new method to measure colors and magnitudes of the tip of the red giant branch in multiple bandpasses simultaneously by fitting an n-dimensional Gaussian to photometry of candidate tip stars. We demonstrate that this method has…

星系天体物理 · 物理学 2020-07-29 M. J. Durbin , R. L. Beaton , J. J. Dalcanton , B. F. Williams , M. L. Boyer

Based on observations from the \emph{FourStar} near-infrared camera on the 6.5m Baade-Magellan telescope at Las Campanas, Chile, we present calibrations of the $JHK$ luminosities of stars defining the tip of the red giant branch (TRGB) in…

The absolute I magnitude of the Tip of the Red Giant Branch M_I(TRGB) is one of the most promising Standard Candles actually used in astrophysics as a fundamental pillar for the Cosmological Distance Scale. With the aim of improving the…

天体物理学 · 物理学 2009-11-06 M. Bellazzini , F. R. Ferraro , E. Pancino

The tip of the red giant (TRGB) is a standardizable candle and is identifiable as the discontinuity at the bright extreme of the red giant branch (RGB) stars in color-magnitude diagram (CMD) space. The TRGB-based distance method has been…

New theoretical evaluations of the Red Giant Branch Tip (TRGB) luminosity, by adopting the most updated physical inputs in computing canonical stellar models, are presented. Theoretical relations for the run of the TRGB bolometric and I…

天体物理学 · 物理学 2015-06-24 M. Salaris , S. Cassisi

The Tip of the Red Giant Branch (TRGB) provides a luminous standard candle for constructing distance ladders to measure the Hubble constant. In practice its measurements via edge-detection response (EDR) are complicated by the apparent…

宇宙学与河外天体物理 · 物理学 2023-04-14 D. Scolnic , A. G. Riess , J. Wu , S. Li , G. S. Anand , R. Beaton , S. Casertano , R. Anderson , S. Dhawan , X. Ke

We use the latest parallaxes measurements from Gaia DR3 to obtain a geometric calibration of the tip of the red giant branch (TRGB) in Cousins $I$ magnitudes as a standard candle for cosmology. We utilise the following surveys: SkyMapper…

星系天体物理 · 物理学 2023-05-24 M. Dixon , J. Mould , C. Flynn , E. N. Taylor , C. Lidman , A. R. Duffy

The absolute bolometric luminosity of the point of core Helium ignition in old, metal poor, red-giant stars is of roughly constant magnitude, varying only very slightly with mass or metallicity. It can thus be used as a standard candle.…

天体物理学 · 物理学 2009-11-10 A. W. McConnachie , M. J. Irwin , A. M. N. Ferguson , R. A. Ibata , G. F. Lewis , N. Tanvir
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