A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Near-infrared spectroscopy of stellar populations in nearby spiral galaxies
Tekijät: Kotilainen JK, Hyvonen T, Reunanen J, Ivanov VD
Kustantaja: WILEY-BLACKWELL
Julkaisuvuosi: 2012
Journal: Monthly Notices of the Royal Astronomical Society
Tietokannassa oleva lehden nimi: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Lehden akronyymi: MON NOT R ASTRON SOC
Numero sarjassa: 2
Vuosikerta: 425
Numero: 2
Aloitussivu: 1057
Lopetussivu: 1067
Sivujen määrä: 11
ISSN: 0035-8711
DOI: https://doi.org/10.1111/j.1365-2966.2012.21425.x
Tiivistelmä
We present high spatial resolution, medium spectral resolution near-infrared (NIR) H- and K-band long-slit spectroscopy for a sample of 29 nearby (z < 0.01) inactive spiral galaxies, to study the composition of their NIR stellar populations. These spectra contain a wealth of diagnostic stellar absorption lines, e.g., Mg?i 1.575?mu m, Si?i 1.588?mu m, CO (63) 1.619?mu m, Mg?i 1.711?mu m, Na?i 2.207?mu m, Ca?i 2.263?mu m and the 12CO and 13CO bandheads longward of 2.29?mu m. We use NIR absorption features to study the stellar population and star formation properties of the spiral galaxies along the Hubble sequence, and we produce the first high spatial resolution NIR HK-band template spectra for low-redshift spiral galaxies along the Hubble sequence. These templates will find applications in a variety of galaxy studies. The strength of the absorption lines depends on the luminosity and/or temperature of stars and, therefore, spectral indices can be used to trace the stellar population of galaxies. The entire sample indicates that the evolved red stars completely dominate the NIR spectra, and that the contribution from hot young stars is insignificant.
We present high spatial resolution, medium spectral resolution near-infrared (NIR) H- and K-band long-slit spectroscopy for a sample of 29 nearby (z < 0.01) inactive spiral galaxies, to study the composition of their NIR stellar populations. These spectra contain a wealth of diagnostic stellar absorption lines, e.g., Mg?i 1.575?mu m, Si?i 1.588?mu m, CO (63) 1.619?mu m, Mg?i 1.711?mu m, Na?i 2.207?mu m, Ca?i 2.263?mu m and the 12CO and 13CO bandheads longward of 2.29?mu m. We use NIR absorption features to study the stellar population and star formation properties of the spiral galaxies along the Hubble sequence, and we produce the first high spatial resolution NIR HK-band template spectra for low-redshift spiral galaxies along the Hubble sequence. These templates will find applications in a variety of galaxy studies. The strength of the absorption lines depends on the luminosity and/or temperature of stars and, therefore, spectral indices can be used to trace the stellar population of galaxies. The entire sample indicates that the evolved red stars completely dominate the NIR spectra, and that the contribution from hot young stars is insignificant.
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