| JANÍK, Jan, Jiří KRTIČKA a Zdeněk MIKULÁŠEK. Is sigma Sculptoris Really a Chemically Peculiar Star? In Kudryavtsev, D. O.; Balega, Yu. Yu.; Romanyuk, I. I. Physics and Evolution of Magnetic and Related Stars. 494. vyd. San Francisco: Astronomical Society of the Pacific, 2015, s. 197-202. ISBN 978-1-58381-872-5. |
Další formáty:
BibTeX
LaTeX
RIS
@inproceedings{1298618,
author = {Janík, Jan and Krtička, Jiří and Mikulášek, Zdeněk},
address = {San Francisco},
booktitle = {Physics and Evolution of Magnetic and Related Stars},
edition = {494},
editor = {Kudryavtsev, D. O.; Balega, Yu. Yu.; Romanyuk, I. I.},
keywords = {sigma Scl; spectroscopy; CP stars},
howpublished = {tištěná verze "print"},
language = {eng},
location = {San Francisco},
isbn = {978-1-58381-872-5},
pages = {197-202},
publisher = {Astronomical Society of the Pacific},
title = {Is sigma Sculptoris Really a Chemically Peculiar Star?},
year = {2015}
}
TY - JOUR
ID - 1298618
AU - Janík, Jan - Krtička, Jiří - Mikulášek, Zdeněk
PY - 2015
TI - Is sigma Sculptoris Really a Chemically Peculiar Star?
PB - Astronomical Society of the Pacific
CY - San Francisco
SN - 9781583818725
KW - sigma Scl
KW - spectroscopy
KW - CP stars
N2 - We have spectroscopically observed the star sigma Scl during two seasons (2011-2012) with the high dispersion spectrograph FEROS (R = 48 000) attached to the 2.2-m MPG/ESO telescope at La Silla. We did not find any spectral changes in a total of 60 obtained spectra. The chemical composition of sigma Scl is very similar to the solar one. We are also unable to find any periodic photometric variations of the star. Consequently, we cannot classify it as a CP star.
ER -
JANÍK, Jan, Jiří KRTIČKA a Zdeněk MIKULÁŠEK. Is sigma Sculptoris Really a Chemically Peculiar Star? In Kudryavtsev, D. O.; Balega, Yu. Yu.; Romanyuk, I. I. \textit{Physics and Evolution of Magnetic and Related Stars}. 494. vyd. San Francisco: Astronomical Society of the Pacific, 2015, s.~197-202. ISBN~978-1-58381-872-5.
|
