| PIECKA, Martin a Ernst PAUNZEN. A Comparison of the Simulations and Observations for a Nearby Spiral Arm. Frontiers in Astronomy and Space Sciences. Frontiers Media SA, 2021, roč. 8, June, s. "642776", 20 s. ISSN 2296-987X. Dostupné z: https://dx.doi.org/10.3389/fspas.2021.642776. |
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@article{1784088,
author = {Piecka, Martin and Paunzen, Ernst},
article_number = {June},
doi = {http://dx.doi.org/10.3389/fspas.2021.642776},
keywords = {galaxy: kinematics and dynamics; galaxy: disc; galaxy: evolution; galaxy: structure; open clusters and associations: general; local interstellar matter},
language = {eng},
issn = {2296-987X},
journal = {Frontiers in Astronomy and Space Sciences},
title = {A Comparison of the Simulations and Observations for a Nearby Spiral Arm},
url = {https://doi.org/10.3389/fspas.2021.642776},
volume = {8},
year = {2021}
}
TY - JOUR
ID - 1784088
AU - Piecka, Martin - Paunzen, Ernst
PY - 2021
TI - A Comparison of the Simulations and Observations for a Nearby Spiral Arm
JF - Frontiers in Astronomy and Space Sciences
VL - 8
IS - June
SP - "642776"
EP - "642776"
PB - Frontiers Media SA
SN - 2296987X
KW - galaxy: kinematics and dynamics
KW - galaxy: disc
KW - galaxy: evolution
KW - galaxy: structure
KW - open clusters and associations: general
KW - local interstellar matter
UR - https://doi.org/10.3389/fspas.2021.642776
N2 - 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.
ER -
PIECKA, Martin a Ernst PAUNZEN. A Comparison of the Simulations and Observations for a Nearby Spiral Arm. \textit{Frontiers in Astronomy and Space Sciences}. Frontiers Media SA, 2021, roč.~8, June, s.~''642776'', 20 s. ISSN~2296-987X. Dostupné z: https://dx.doi.org/10.3389/fspas.2021.642776.
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