PIECKA, Martin and Ernst PAUNZEN. A Comparison of the Simulations and Observations for a Nearby Spiral Arm. Frontiers in Astronomy and Space Sciences. Frontiers Media SA, 2021, vol. 8, June, p. "642776", 20 pp. ISSN 2296-987X. Available from: https://dx.doi.org/10.3389/fspas.2021.642776.
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Basic information
Original name A Comparison of the Simulations and Observations for a Nearby Spiral Arm
Authors PIECKA, Martin (703 Slovakia, belonging to the institution) and Ernst PAUNZEN (40 Austria, guarantor, belonging to the institution).
Edition Frontiers in Astronomy and Space Sciences, Frontiers Media SA, 2021, 2296-987X.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Switzerland
Confidentiality degree is not subject to a state or trade secret
WWW URL
Impact factor Impact factor: 4.055
RIV identification code RIV/00216224:14310/21:00122002
Organization unit Faculty of Science
Doi http://dx.doi.org/10.3389/fspas.2021.642776
UT WoS 000668346400001
Keywords in English galaxy: kinematics and dynamics; galaxy: disc; galaxy: evolution; galaxy: structure; open clusters and associations: general; local interstellar matter
Tags rivok
Tags International impact, Reviewed
Changed by Changed by: Mgr. Marie Šípková, DiS., učo 437722. Changed: 28/7/2021 14:58.
Abstract
The analysis is focused on the ability of galactic open clusters to trace the spiral arms, based on the recent data releases from Gaia. For this, a simple 1D description of the motion of spiral arms and clusters is introduced. As next step, results are verified using a widely accepted kinematic model of the motion in spiral galaxies. As expected, both approaches show that open clusters older than about 100 Myr are bad tracers of spiral arms. The younger clusters (ideally < 30 Myr) should be used instead. This agrees with the most recent observational evidence. The latest maps of the diffuse interstellar bands are compared with the spiral structure of the Milky Way and the Antennae Galaxies. The idea of these bands being useful for studying a galactic structure cannot be supported based on the current data.
Links
MUNI/A/1206/2020, interní kód MUName: Pokročilý výzkum v oblasti astrofyziky, teoretické fyziky a fyzikálního vzdělávání
Investor: Masaryk University
MUNI/A/1482/2019, interní kód MUName: Podpora studentského výzkumu v oblasti teoretické fyziky a astrofyziky
Investor: Masaryk University, Category A
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