The R136 star cluster dissected with Hubble Space Telescope/STIS: III. The most massive stars and their clumped winds

Methods. We simultaneously analyse optical and ultraviolet spectroscopy of 53 O-type and three WNh-stars using the FASTWIND model atmosphere code and a genetic algorithm. The models account for optically thick clumps and effects related to porosity and velocity-porosity, as well as a non-void interc...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Brands, Sarah A. (VerfasserIn) , de Koter, Alex (VerfasserIn) , Bestenlehner, Joachim M. (VerfasserIn) , Crowther, Paul A. (VerfasserIn) , Sundqvist, Jon O. (VerfasserIn) , Puls, Joachim (VerfasserIn) , Caballero-Nieves, Saida M. (VerfasserIn) , Abdul-Masih, Michael (VerfasserIn) , Driessen, Florian A. (VerfasserIn) , García, Miriam (VerfasserIn) , Geen, Sam (VerfasserIn) , Gräfener, Götz (VerfasserIn) , Hawcroft, Calum (VerfasserIn) , Kaper, Lex (VerfasserIn) , Keszthelyi, Zsolt (VerfasserIn) , Langer, Norbert (VerfasserIn) , Sana, Hugues (VerfasserIn) , Schneider, Fabian (VerfasserIn) , Shenar, Tomer (VerfasserIn) , Vink, Jorick S. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 19 July 2022
In: Astronomy and astrophysics
Year: 2022, Jahrgang: 663, Pages: 1-44
ISSN:1432-0746
DOI:10.1051/0004-6361/202142742
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.1051/0004-6361/202142742
Verlag, kostenfrei, Volltext: https://www.aanda.org/10.1051/0004-6361/202142742
Volltext
Verfasserangaben:Sarah A. Brands, Alex de Koter, Joachim M. Bestenlehner, Paul A. Crowther, Jon O. Sundqvist, Joachim Puls, Saida M. Caballero-Nieves, Michael Abdul-Masih, Florian A. Driessen, Miriam García, Sam Geen, Götz Gräfener, Calum Hawcroft, Lex Kaper, Zsolt Keszthelyi, Norbert Langer, Hugues Sana, Fabian R. N. Schneider, Tomer Shenar, and Jorick S. Vink

MARC

LEADER 00000caa a2200000 c 4500
001 1816987697
003 DE-627
005 20230118144828.0
007 cr uuu---uuuuu
008 220920s2022 xx |||||o 00| ||eng c
024 7 |a 10.1051/0004-6361/202142742  |2 doi 
035 |a (DE-627)1816987697 
035 |a (DE-599)KXP1816987697 
035 |a (OCoLC)1361696062 
040 |a DE-627  |b ger  |c DE-627  |e rda 
041 |a eng 
084 |a 29  |2 sdnb 
100 1 |a Brands, Sarah A.  |e VerfasserIn  |0 (DE-588)1268466875  |0 (DE-627)181699278X  |4 aut 
245 1 4 |a The R136 star cluster dissected with Hubble Space Telescope/STIS  |b III. The most massive stars and their clumped winds  |c Sarah A. Brands, Alex de Koter, Joachim M. Bestenlehner, Paul A. Crowther, Jon O. Sundqvist, Joachim Puls, Saida M. Caballero-Nieves, Michael Abdul-Masih, Florian A. Driessen, Miriam García, Sam Geen, Götz Gräfener, Calum Hawcroft, Lex Kaper, Zsolt Keszthelyi, Norbert Langer, Hugues Sana, Fabian R. N. Schneider, Tomer Shenar, and Jorick S. Vink 
264 1 |c 19 July 2022 
300 |a 44 
336 |a Text  |b txt  |2 rdacontent 
337 |a Computermedien  |b c  |2 rdamedia 
338 |a Online-Ressource  |b cr  |2 rdacarrier 
500 |a Gesehen am 20.9.2022 
520 |a Methods. We simultaneously analyse optical and ultraviolet spectroscopy of 53 O-type and three WNh-stars using the FASTWIND model atmosphere code and a genetic algorithm. The models account for optically thick clumps and effects related to porosity and velocity-porosity, as well as a non-void interclump medium. - Results. We obtain stellar parameters, surface abundances, mass-loss rates, terminal velocities, and clumping characteristics and compare them to theoretical predictions and evolutionary models. The clumping properties include the density of the interclump medium and the velocity-porosity of the wind. For the first time, these characteristics are systematically measured for a wide range of effective temperatures and luminosities. - Conclusions. We confirm a cluster age of 1.0-2.5 Myr and derived an initial stellar mass of ≥250 M for the most massive star in our sample, R136a1. The winds of our sample stars are highly clumped, with an average clumping factor of fcl = 29 ± 15. We find tentative trends in the wind-structure parameters as a function of the mass-loss rate, suggesting that the winds of stars with higher mass-loss rates are less clumped. We compare several theoretical predictions to the observed mass-loss rates and terminal velocities and find that none satisfactorily reproduce both quantities. The prescription of Krticˇka & Kubát (2018) matches the observed mass-loss rates best. 
700 1 |a de Koter, Alex  |e VerfasserIn  |4 aut 
700 1 |a Bestenlehner, Joachim M.  |e VerfasserIn  |4 aut 
700 1 |a Crowther, Paul A.  |e VerfasserIn  |4 aut 
700 1 |a Sundqvist, Jon O.  |e VerfasserIn  |4 aut 
700 1 |a Puls, Joachim  |e VerfasserIn  |4 aut 
700 1 |a Caballero-Nieves, Saida M.  |e VerfasserIn  |4 aut 
700 1 |a Abdul-Masih, Michael  |e VerfasserIn  |4 aut 
700 1 |a Driessen, Florian A.  |e VerfasserIn  |4 aut 
700 1 |a García, Miriam  |e VerfasserIn  |4 aut 
700 1 |a Geen, Sam  |e VerfasserIn  |4 aut 
700 1 |a Gräfener, Götz  |e VerfasserIn  |4 aut 
700 1 |a Hawcroft, Calum  |e VerfasserIn  |4 aut 
700 1 |a Kaper, Lex  |e VerfasserIn  |4 aut 
700 1 |a Keszthelyi, Zsolt  |e VerfasserIn  |4 aut 
700 1 |a Langer, Norbert  |e VerfasserIn  |4 aut 
700 1 |a Sana, Hugues  |e VerfasserIn  |4 aut 
700 1 |a Schneider, Fabian  |e VerfasserIn  |0 (DE-588)1069401307  |0 (DE-627)821861212  |0 (DE-576)42867223X  |4 aut 
700 1 |a Shenar, Tomer  |e VerfasserIn  |4 aut 
700 1 |a Vink, Jorick S.  |e VerfasserIn  |4 aut 
773 0 8 |i Enthalten in  |t Astronomy and astrophysics  |d Les Ulis : EDP Sciences, 1969  |g 663(2022), Artikel-ID A36, Seite 1-44  |h Online-Ressource  |w (DE-627)253390222  |w (DE-600)1458466-9  |w (DE-576)072283351  |x 1432-0746  |7 nnas  |a The R136 star cluster dissected with Hubble Space Telescope/STIS III. The most massive stars and their clumped winds 
773 1 8 |g volume:663  |g year:2022  |g elocationid:A36  |g pages:1-44  |g extent:44  |a The R136 star cluster dissected with Hubble Space Telescope/STIS III. The most massive stars and their clumped winds 
856 4 0 |u https://doi.org/10.1051/0004-6361/202142742  |x Verlag  |x Resolving-System  |z kostenfrei  |3 Volltext 
856 4 0 |u https://www.aanda.org/10.1051/0004-6361/202142742  |x Verlag  |z kostenfrei  |3 Volltext 
951 |a AR 
992 |a 20220920 
993 |a Article 
994 |a 2022 
998 |g 1069401307  |a Schneider, Fabian  |m 1069401307:Schneider, Fabian  |d 700000  |d 714000  |d 700000  |d 728500  |e 700000PS1069401307  |e 714000PS1069401307  |e 700000PS1069401307  |e 728500PS1069401307  |k 0/700000/  |k 1/700000/714000/  |k 0/700000/  |k 1/700000/728500/  |p 18 
999 |a KXP-PPN1816987697  |e 4190191825 
BIB |a Y 
SER |a journal 
JSO |a {"title":[{"subtitle":"III. The most massive stars and their clumped winds","title":"The R136 star cluster dissected with Hubble Space Telescope/STIS","title_sort":"R136 star cluster dissected with Hubble Space Telescope/STIS"}],"person":[{"display":"Brands, Sarah A.","family":"Brands","roleDisplay":"VerfasserIn","given":"Sarah A.","role":"aut"},{"role":"aut","given":"Alex","display":"de Koter, Alex","family":"de Koter","roleDisplay":"VerfasserIn"},{"given":"Joachim M.","role":"aut","family":"Bestenlehner","display":"Bestenlehner, Joachim M.","roleDisplay":"VerfasserIn"},{"given":"Paul A.","role":"aut","roleDisplay":"VerfasserIn","family":"Crowther","display":"Crowther, Paul A."},{"given":"Jon O.","role":"aut","roleDisplay":"VerfasserIn","display":"Sundqvist, Jon O.","family":"Sundqvist"},{"given":"Joachim","role":"aut","display":"Puls, Joachim","family":"Puls","roleDisplay":"VerfasserIn"},{"role":"aut","given":"Saida M.","display":"Caballero-Nieves, Saida M.","family":"Caballero-Nieves","roleDisplay":"VerfasserIn"},{"roleDisplay":"VerfasserIn","display":"Abdul-Masih, Michael","family":"Abdul-Masih","role":"aut","given":"Michael"},{"display":"Driessen, Florian A.","family":"Driessen","roleDisplay":"VerfasserIn","role":"aut","given":"Florian A."},{"display":"García, Miriam","family":"García","roleDisplay":"VerfasserIn","role":"aut","given":"Miriam"},{"given":"Sam","role":"aut","family":"Geen","display":"Geen, Sam","roleDisplay":"VerfasserIn"},{"role":"aut","given":"Götz","display":"Gräfener, Götz","family":"Gräfener","roleDisplay":"VerfasserIn"},{"role":"aut","given":"Calum","family":"Hawcroft","display":"Hawcroft, Calum","roleDisplay":"VerfasserIn"},{"role":"aut","given":"Lex","roleDisplay":"VerfasserIn","family":"Kaper","display":"Kaper, Lex"},{"given":"Zsolt","role":"aut","display":"Keszthelyi, Zsolt","family":"Keszthelyi","roleDisplay":"VerfasserIn"},{"given":"Norbert","role":"aut","display":"Langer, Norbert","family":"Langer","roleDisplay":"VerfasserIn"},{"given":"Hugues","role":"aut","display":"Sana, Hugues","family":"Sana","roleDisplay":"VerfasserIn"},{"roleDisplay":"VerfasserIn","family":"Schneider","display":"Schneider, Fabian","role":"aut","given":"Fabian"},{"role":"aut","given":"Tomer","roleDisplay":"VerfasserIn","display":"Shenar, Tomer","family":"Shenar"},{"given":"Jorick S.","role":"aut","roleDisplay":"VerfasserIn","display":"Vink, Jorick S.","family":"Vink"}],"note":["Gesehen am 20.9.2022"],"type":{"bibl":"article-journal","media":"Online-Ressource"},"physDesc":[{"extent":"44 S."}],"language":["eng"],"id":{"doi":["10.1051/0004-6361/202142742"],"eki":["1816987697"]},"recId":"1816987697","relHost":[{"part":{"volume":"663","year":"2022","pages":"1-44","text":"663(2022), Artikel-ID A36, Seite 1-44","extent":"44"},"name":{"displayForm":["European Southern Observatory (ESO)"]},"corporate":[{"roleDisplay":"Herausgebendes Organ","display":"European Southern Observatory","role":"isb"}],"origin":[{"dateIssuedDisp":"1969-","publisher":"EDP Sciences ; Springer","publisherPlace":"Les Ulis ; Berlin ; Heidelberg","dateIssuedKey":"1969"}],"disp":"The R136 star cluster dissected with Hubble Space Telescope/STIS III. The most massive stars and their clumped windsAstronomy and astrophysics","pubHistory":["1.1969 -"],"type":{"media":"Online-Ressource","bibl":"periodical"},"note":["Gesehen am 21.06.2024","Erscheint 36mal jährlich in 12 Bänden zu je 3 Ausgaben","Fortsetzung der Druck-Ausgabe"],"title":[{"subtitle":"an international weekly journal","title":"Astronomy and astrophysics","title_sort":"Astronomy and astrophysics"}],"recId":"253390222","titleAlt":[{"title":"Astronomy & astrophysics"},{"title":"a European journal"}],"language":["eng"],"id":{"zdb":["1458466-9"],"issn":["1432-0746"],"eki":["253390222"]},"physDesc":[{"extent":"Online-Ressource"}]}],"name":{"displayForm":["Sarah A. Brands, Alex de Koter, Joachim M. Bestenlehner, Paul A. Crowther, Jon O. Sundqvist, Joachim Puls, Saida M. Caballero-Nieves, Michael Abdul-Masih, Florian A. Driessen, Miriam García, Sam Geen, Götz Gräfener, Calum Hawcroft, Lex Kaper, Zsolt Keszthelyi, Norbert Langer, Hugues Sana, Fabian R. N. Schneider, Tomer Shenar, and Jorick S. Vink"]},"origin":[{"dateIssuedDisp":"19 July 2022","dateIssuedKey":"2022"}]} 
SRT |a BRANDSSARAR136STARCL1920