Stars with Discrepant v sin i as Derived from the Ca II 3933 and Mg II 4481 angstrom Lines. VII. HD 9531 (SB), HD 31592 (SB2), HD 129174 (SB?)

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F18%3A00113395" target="_blank" >RIV/00216224:14310/18:00113395 - isvavai.cz</a>

Výsledek na webu

<a href="https://link.springer.com/article/10.1134%2FS1990341318030094" target="_blank" >https://link.springer.com/article/10.1134%2FS1990341318030094</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1134/S1990341318030094" target="_blank" >10.1134/S1990341318030094</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Stars with Discrepant v sin i as Derived from the Ca II 3933 and Mg II 4481 angstrom Lines. VII. HD 9531 (SB), HD 31592 (SB2), HD 129174 (SB?)

Popis výsledku v původním jazyce

In this paper of the series we analyze three stars listed among stars with discrepant v sin i: HD 9531 and HD 31592, which also show radial velocity variations inherent to spectroscopic binaries, and HD 129174 which is an Mn-type star with a possible magnetic field. In HD 9531 we confirm the radial velocity derived from the hydrogen lines as well as from the Ca II line at 3933 angstrom as variable. The profile of the calcium line also appears variable, and with the estimated magnetic induction B-e = -630 +/- 1340 G, this suggests that the abundance of calcium possibly varies over the surface of the star. We identified the lines of the secondary component in the spectrum of HD 31592 revealing thus it is an SB2 binary with B9.5V and A0V components. While the primary star rotates with v sin i = 50 km s(-1), the secondary star is faster with v sin i = 170 km s(-1). We find that only 60% of the Mn lines identified in the spectrum of HD 129174 can be fitted with a unique abundance value, whereas the remaining lines are stronger or fainter. We also identified two Xe II lines at 5339.33 angstrom and 5419.15 angstrom and estimated their log g f.

Název v anglickém jazyce

Stars with Discrepant v sin i as Derived from the Ca II 3933 and Mg II 4481 angstrom Lines. VII. HD 9531 (SB), HD 31592 (SB2), HD 129174 (SB?)

Popis výsledku anglicky

In this paper of the series we analyze three stars listed among stars with discrepant v sin i: HD 9531 and HD 31592, which also show radial velocity variations inherent to spectroscopic binaries, and HD 129174 which is an Mn-type star with a possible magnetic field. In HD 9531 we confirm the radial velocity derived from the hydrogen lines as well as from the Ca II line at 3933 angstrom as variable. The profile of the calcium line also appears variable, and with the estimated magnetic induction B-e = -630 +/- 1340 G, this suggests that the abundance of calcium possibly varies over the surface of the star. We identified the lines of the secondary component in the spectrum of HD 31592 revealing thus it is an SB2 binary with B9.5V and A0V components. While the primary star rotates with v sin i = 50 km s(-1), the secondary star is faster with v sin i = 170 km s(-1). We find that only 60% of the Mn lines identified in the spectrum of HD 129174 can be fitted with a unique abundance value, whereas the remaining lines are stronger or fainter. We also identified two Xe II lines at 5339.33 angstrom and 5419.15 angstrom and estimated their log g f.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2018

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Astrophysical Bulletin

ISSN

1990-3413

e-ISSN

—

Svazek periodika

73

Číslo periodika v rámci svazku

3

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

12

Strana od-do

351-362

Kód UT WoS článku

000444442700009

EID výsledku v databázi Scopus

2-s2.0-85053179257