High-Resolution Spectroscopy for Cepheids Distance Determination. I. Line Asymmetry.

Nardetto, N., Mourard, D., Kervella, P., Mathias, P., Mérand, A., & Bersier, D. (2006). High-Resolution Spectroscopy for Cepheids Distance Determination. I. Line Asymmetry. Astronomy & Astrophysics, 309-319.

Type

Journal article

Intellectual base

Primary research

Year

2006

DOI

10.1051/0004-6361:20054333

Link

https://doi.org/10.1051/0004-6361:20054333

Cited by

1 citation across 1 artifact.

Domain-specific

• Baade–Wesselink Method
  • In practice, (p) is not a trivial geometric constant: limb darkening, velocity gradients, line formation, cross-correlation procedure, and the chosen photospheric layer contribute to it.

Verification

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Registry ID ref:0ed36080a769 · see in the full table