HST viewing of spectacular star-forming trails behind ESO 137-001

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00573496" target="_blank" >RIV/67985815:_____/23:00573496 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1093/mnras/stad963" target="_blank" >https://doi.org/10.1093/mnras/stad963</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stad963" target="_blank" >10.1093/mnras/stad963</a>

Result language
angličtina
Original language name
HST viewing of spectacular star-forming trails behind ESO 137-001
Original language description
We present the results from the HST WFC3 and ACS data on an archetypal galaxy undergoing ram pressure stripping (RPS), ESO 137-001, in the nearby cluster Abell 3627. ESO 137-001 is known to host a prominent stripped tail detected in many bands from X-rays, H α to CO. The HST data reveal significant features indicative of RPS such as asymmetric dust distribution and surface brightness as well as many blue young star complexes in the tail. We study the correlation between the blue young star complexes from HST, H II regions from H α (MUSE), and dense molecular clouds from CO (ALMA).
Czech name
—
Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/LM2023059" target="_blank" >LM2023059: Atacama Large Millimeter /submillimeter Array – participation of the Czech Republic</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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