On the near infrared variability of chemically peculiar stars
| dc.creator | Catalano, F. A. | |
| dc.creator | Leone, F. | |
| dc.date | 1998-05-06 | |
| dc.date.accessioned | 2026-07-07T02:26:50Z | |
| dc.date.available | 2026-07-07T02:26:50Z | |
| dc.description | Some CP stars have recently been discovered by Catalano et al. (1991) to be variable also in the near infrared, although with smaller amplitudes than in the visible. Hence an observational campaign was started in which the infrared light variability of a number of CP2 and CP4 stars has been investigated at the ESO-La Silla Observatory in the bands J, H, and K. As a general result, infrared variations show the same behavior in all three filters but amplitudes are smaller than in the visible. | |
| dc.description | 3 pages, no figure, to appear in: Proc. of the 26th workshop of the European Working Group on CP stars, eds. P. North, A. Schnell and J. Ziznovsky, Contrib. Astr. Obs. Skalnate Pleso Vol. 27, No 3 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9805072 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9805072 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12439 | |
| dc.subject | Astrophysics | |
| dc.title | On the near infrared variability of chemically peculiar stars | |
| dc.type | text |