We have investigated how the K-band magnitude of the red clump $[M_K(RC)]$ depends on age and metallicity, using 2MASS infrared data for a sample of 24 open clusters with known distances. We show that a constant value of $M_K(RC)=-1.57 \pm 0.05$ is a reasonable assumption to use in distance determinations for clusters with metallicity between -0.5 and +0.4 dex and age between 108.5 and 109.9 years
This study presents the multiwavelength investigation of the absolute magnitudes and colors of the r...
We have obtained spectra with a resolution of similar to2.5 Angstrom in the region of approximate to...
We present infrared observations for more than 100 red giants and clump stars in eight old open clus...
We present a detailed analysis of the behaviour of the Red Clump K-band absolute magnitude (M(K,RC))...
Context. Over the past decade the use of the red clump (RC) as distance indicator has increased in ...
We use near-infrared observations of eight selected Galactic globular clusters to estimate their dis...
We present an M-V absolute magnitude calibration including the B - V colour and [Fe/H] metallicity f...
We present distance modulus and reddening determinations for 72 Galactic globular clusters from the ...
We present distance modulus and reddening determinations for 72 Galactic globular clusters from the ...
Red clump stars are fundamental distance indicators in astrophysics, although theoretical stellar mo...
We present distance modulus and reddening determinations for 72 Galactic globular clusters from the ...
We present the analysis of the color-magnitude relation (CMR) for a sample of 57 X-ray detected Abel...
We present a detailed analysis of the uncertainty on the theoretical population corrections to the L...
We analyze the UBVI color-magnitude diagrams of a relatively low-reddening region of Baade's Window....
The tip of the red giant branch (TRGB) is a well-established standard candle used to measure distanc...
This study presents the multiwavelength investigation of the absolute magnitudes and colors of the r...
We have obtained spectra with a resolution of similar to2.5 Angstrom in the region of approximate to...
We present infrared observations for more than 100 red giants and clump stars in eight old open clus...
We present a detailed analysis of the behaviour of the Red Clump K-band absolute magnitude (M(K,RC))...
Context. Over the past decade the use of the red clump (RC) as distance indicator has increased in ...
We use near-infrared observations of eight selected Galactic globular clusters to estimate their dis...
We present an M-V absolute magnitude calibration including the B - V colour and [Fe/H] metallicity f...
We present distance modulus and reddening determinations for 72 Galactic globular clusters from the ...
We present distance modulus and reddening determinations for 72 Galactic globular clusters from the ...
Red clump stars are fundamental distance indicators in astrophysics, although theoretical stellar mo...
We present distance modulus and reddening determinations for 72 Galactic globular clusters from the ...
We present the analysis of the color-magnitude relation (CMR) for a sample of 57 X-ray detected Abel...
We present a detailed analysis of the uncertainty on the theoretical population corrections to the L...
We analyze the UBVI color-magnitude diagrams of a relatively low-reddening region of Baade's Window....
The tip of the red giant branch (TRGB) is a well-established standard candle used to measure distanc...
This study presents the multiwavelength investigation of the absolute magnitudes and colors of the r...
We have obtained spectra with a resolution of similar to2.5 Angstrom in the region of approximate to...
We present infrared observations for more than 100 red giants and clump stars in eight old open clus...