A SPECTRAL ATLAS OF lambda BOOTIS STARS

J 2014

A SPECTRAL ATLAS OF lambda BOOTIS STARS

PAUNZEN, Ernst a Ulrike HEITER

Základní údaje

Originální název

A SPECTRAL ATLAS OF lambda BOOTIS STARS

Autoři

PAUNZEN, Ernst (40 Rakousko, garant, domácí) a Ulrike HEITER (752 Švédsko)

Vydání

SERBIAN ASTRONOMICAL JOURNAL, BELGRADE, ASTRONOMICAL OBSERVATORY BELGRADE, 2014, 1450-698X

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Srbsko

Utajení

není předmětem státního či obchodního tajemství

Impakt faktor

Impact factor: 0.704

Kód RIV

RIV/00216224:14310/14:00076701

Organizační jednotka

Přírodovědecká fakulta

DOI

http://dx.doi.org/10.2298/SAJ1488075P

UT WoS

000340034400008

Klíčová slova anglicky

atlases; stars: chemically peculiar; stars: fundamental parameters

Štítky

AKR, rivok

Změněno: 3. 10. 2014 11:40, doc. Ernst Paunzen, Dr.rer.nat

Anotace

V originále

AB Since the discovery of lambda Bootis stars, a permanent confusion about their classification can be found in literature. This group of non-magnetic, Population I, metal-poor A to F-type stars, has often been used as some sort of trash can for "exotic" and spectroscopically dubious objects. Some attempts have been made to establish a homogeneous group of stars which share the same common properties. Unfortunately, the flood of "new" information (e.g. UV and IR data) led again to a whole zoo of objects classified as lambda Bootis stars, which, however, are apparent non-members. To overcome this unsatisfying situation, a spectral atlas of well established lambda Bootis stars for the classical optical domain was compiled. It includes intermediate dispersion (40 and 120 Angstroem/mm) spectra of three lambda Bootis, as well as appropriate MK standard stars. Furthermore, "suspicious" objects, such as shell and Field Horizontal Branch stars, have been considered in order to provide to classifiers a homogeneous reference. As a further step, a high resolution (8 Angstroem/mm) spectrum of one "classical" lambda Bootis star in the same wavelength region (3800 - 4600 Angstroem) is presented. In total, 55 lines can be used for this particular star to derive detailed abundances for nine heavy elements (Mg, Ca, Sc, Ti, Cr, Mn, Fe, Sr and Ba).

Návaznosti

3SGA5916, interní kód MU

Název: Hvězdy a hvězdokupy v Magellanových mračnech (Akronym: Webda MaC)

Investor: Jihomoravský kraj, Hvězdy a hvězdokupy v Magellanových mračnech, Granty pro zahraniční vědce

7AMB14AT015, projekt VaV

Název: Nový pohled na magnetické hvězdy (Akronym: MAGSTARS)

Investor: Ministerstvo školství, mládeže a tělovýchovy ČR, Nový pohled na magnetické hvězdy

Citovat

PAUNZEN, Ernst a Ulrike HEITER. A SPECTRAL ATLAS OF lambda BOOTIS STARS. SERBIAN ASTRONOMICAL JOURNAL. BELGRADE: ASTRONOMICAL OBSERVATORY BELGRADE, 2014, roč. 188, č. 6, s. 75-84. ISSN 1450-698X. Dostupné z: https://dx.doi.org/10.2298/SAJ1488075P.

@article{1200176,
   author = {Paunzen, Ernst and Heiter, Ulrike},
   article_location = {BELGRADE},
   article_number = {6},
   doi = {http://dx.doi.org/10.2298/SAJ1488075P},
   keywords = {atlases; stars: chemically peculiar; stars: fundamental parameters},
   language = {eng},
   issn = {1450-698X},
   journal = {SERBIAN ASTRONOMICAL JOURNAL},
   title = {A SPECTRAL ATLAS OF lambda BOOTIS STARS},
   volume = {188},
   year = {2014}
}

TY  - JOUR
ID  - 1200176
AU  - Paunzen, Ernst - Heiter, Ulrike
PY  - 2014
TI  - A SPECTRAL ATLAS OF lambda BOOTIS STARS
JF  - SERBIAN ASTRONOMICAL JOURNAL
VL  - 188
IS  - 6
SP  - 75-84
EP  - 75-84
PB  - ASTRONOMICAL OBSERVATORY BELGRADE
SN  - 1450698X
KW  - atlases
KW  - stars: chemically peculiar
KW  - stars: fundamental parameters
N2  - AB Since the discovery of lambda Bootis stars, a permanent confusion about their classification can be found in literature. This group of non-magnetic, Population I, metal-poor A to F-type stars, has often been used as some sort of trash can for "exotic" and spectroscopically dubious objects. Some attempts have been made to establish a homogeneous group of stars which share the same common properties. Unfortunately, the flood of "new" information (e.g. UV and IR data) led again to a whole zoo of objects classified as lambda Bootis stars, which, however, are apparent non-members. To overcome this unsatisfying situation, a spectral atlas of well established lambda Bootis stars for the classical optical domain was compiled. It includes intermediate dispersion (40 and 120 Angstroem/mm) spectra of three lambda Bootis, as well as appropriate MK standard stars. Furthermore, "suspicious" objects, such as shell and Field Horizontal Branch stars, have been considered in order to provide to classifiers a homogeneous reference. As a further step, a high resolution (8 Angstroem/mm) spectrum of one "classical" lambda Bootis star in the same wavelength region (3800 - 4600 Angstroem) is presented. In total, 55 lines can be used for this particular star to derive detailed abundances for nine heavy elements (Mg, Ca, Sc, Ti, Cr, Mn, Fe, Sr and Ba).
ER  -

PAUNZEN, Ernst a Ulrike HEITER. A SPECTRAL ATLAS OF lambda BOOTIS STARS. \textit{SERBIAN ASTRONOMICAL JOURNAL}. BELGRADE: ASTRONOMICAL OBSERVATORY BELGRADE, 2014, roč.~188, č.~6, s.~75-84. ISSN~1450-698X. Dostupné z: https://dx.doi.org/10.2298/SAJ1488075P.

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