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The GALAH survey : new diffuse interstellar bands found in residuals of 872 000 stellar spectra
ID
Vogrinčič, Rok
(
Avtor
),
ID
Kos, Janez
(
Avtor
),
ID
Zwitter, Tomaž
(
Avtor
),
ID
Traven, Gregor
(
Avtor
),
ID
Beeson, Kevin Luke
(
Avtor
),
ID
Čotar, Klemen
(
Avtor
), et al.
PDF - Predstavitvena datoteka,
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MD5: F4DF3D3FAD4B6559564A20458D9B9511
URL - Izvorni URL, za dostop obiščite
https://academic.oup.com/mnras/article/521/3/3727/7085973
Galerija slik
Izvleček
We use more than 872 000 mid- to high-resolution (R ∼ 20 000) spectra of stars from the GALactic Archaeology with HERMES (GALAH) survey to discern the spectra of diffuse interstellar bands (DIBs). We use four windows with the wavelength ranges 4718–4903, 5649–5873, 6481–6739, and 7590–7890 Å, giving a total coverage of 967 Å. We produce ∼400 000 spectra of interstellar medium (ISM) absorption features and correct them for radial velocities of the DIB clouds. Ultimately, we combine the 33 115 best ISM spectra into six reddening bins with a range of 0.1 < E(B − V) < 0.7 mag. A total of 183 absorption features in these spectra qualify as DIBs, and their fitted model parameters are summarized in a detailed catalogue. From these, 64 are not reported in the literature, of which 17 are certain, 14 are probable and 33 are possible. We find that the broad DIBs can be fitted with a multitude of narrower DIBs. Finally, we create a synthetic DIB spectrum at unit reddening. This should allow us to narrow down the possible carriers of DIBs, to explore the composition of the ISM, and ultimately to model dust and star formation better as well as to correct Galactic and extragalactic observations. The majority of certain DIBs show a significant excess of equivalent width when compared with reddening. We explain this with observed lines of sight penetrating more uniform DIB clouds compared with clumpy dust clouds.
Jezik:
Angleški jezik
Ključne besede:
catalogues
,
spectroscopic surveys
,
methods
,
data analysis
,
surveys
,
dust
,
extinction
Vrsta gradiva:
Članek v reviji
Tipologija:
1.01 - Izvirni znanstveni članek
Organizacija:
FMF - Fakulteta za matematiko in fiziko
Status publikacije:
Objavljeno
Različica publikacije:
Objavljena publikacija
Leto izida:
2023
Št. strani:
Str. 3727-3748
Številčenje:
Vol. 521, iss. 3
PID:
20.500.12556/RUL-147271
UDK:
524.3
ISSN pri članku:
1365-2966
DOI:
10.1093/mnras/stad678
COBISS.SI-ID:
152621827
Datum objave v RUL:
28.06.2023
Število ogledov:
603
Število prenosov:
56
Metapodatki:
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Objavi na:
Gradivo je del revije
Naslov:
Monthly notices of the Royal Astronomical Society
Skrajšan naslov:
Mon. not. R. Astron. Soc.
Založnik:
Blackwell Science
ISSN:
1365-2966
COBISS.SI-ID:
1870180
Licence
Licenca:
CC BY 4.0, Creative Commons Priznanje avtorstva 4.0 Mednarodna
Povezava:
http://creativecommons.org/licenses/by/4.0/deed.sl
Opis:
To je standardna licenca Creative Commons, ki daje uporabnikom največ možnosti za nadaljnjo uporabo dela, pri čemer morajo navesti avtorja.
Projekti
Financer:
ARRS - Agencija za raziskovalno dejavnost Republike Slovenije
Številka projekta:
P1-0188
Naslov:
Astrofizika in fizika atmosfere
Financer:
ARC - Australian Research Council
Številka projekta:
CE170100013
Naslov:
Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions
Akronim:
ASTRO 3D
Financer:
ARC - Australian Research Council
Program financ.:
Discovery Projects
Številka projekta:
DP180101791
Financer:
Drugi - Drug financer ali več financerjev
Program financ.:
UNSW, Scientia Fellowship
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