| | |
| | |
Stat |
Members: 3643 Articles: 2'488'730 Articles rated: 2609
29 March 2024 |
|
| | | |
|
Article overview
| |
|
Updated pulsation models for anomalous Cepheids | M. Marconi
; G. Fiorentino
; F. Caputo
; | Date: |
16 Dec 2003 | Journal: | Astron.Astrophys. 417 (2004) 1101-1114 | Subject: | astro-ph | Affiliation: | INAF - Astron. Obs. of Capodimonte), G. Fiorentino (University of Tor Vergata, Roma), F. Caputo (INAF - Astron. Obs. of Roma | Abstract: | A theoretical investigation of the pulsation behavior of so-named ``anomalous’’ Cepheids is presented. The study is based on nonlinear convective pulsation models with $Z$=0.0001 and 0.0004, mass in the range 1.3-2.2 Mo and various luminosity levels. Based on these computations, we derive period, bolometric light curves and the edges of the instability strip, showing that a variation of the metal abundance from Z=0.0001 to 0.0004 has quite small effects on these quantities. Then, using bolometric corrections and color-temperature transformations, we are able to provide the predicted relations connecting pulsational properties (periods, amplitudes) with magnitudes and colors in the various photometric bands. The theoretical pulsational scenario is compared to observed anomalous Cepheids in dwarf spheroidal galaxies and, in particular, the predicted mass-dependent Period-Magnitude-Amplitude and Period-Magnitude-Color relations are used to estimate individual mass values, as well as to discriminate between fundamental (F) and first-overtone (FO) pulsators. | Source: | arXiv, astro-ph/0401332 | Services: | Forum | Review | PDF | Favorites |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser claudebot
|
| |
|
|
|
| News, job offers and information for researchers and scientists:
| |