A comparison of X-ray and strong lensing properties of simulated X-ray clusters
We use gas-dynamical simulations of galaxy clusters to compare their X-ray and strong lensing properties. Special emphasis is laid on mass estimates. The cluster masses range between 6 x 10^14 solar masses and 4 x 10^15 solar masses, and they are examined at redshifts between 1 and 0. We compute the...
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
19 Mar 1996
|
| In: |
Arxiv
|
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/astro-ph/9603101
|
| Verfasserangaben: | Matthias Bartelmann and Matthias Steinmetz |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1563969157 | ||
| 003 | DE-627 | ||
| 005 | 20220813232940.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 170929s1996 xx |||||o 00| ||eng c | ||
| 035 | |a (DE-627)1563969157 | ||
| 035 | |a (DE-576)493969152 | ||
| 035 | |a (DE-599)BSZ493969152 | ||
| 035 | |a (OCoLC)1340979675 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Bartelmann, Matthias |d 1965- |e VerfasserIn |0 (DE-588)141554185 |0 (DE-627)629953090 |0 (DE-576)170611779 |4 aut | |
| 245 | 1 | 2 | |a A comparison of X-ray and strong lensing properties of simulated X-ray clusters |c Matthias Bartelmann and Matthias Steinmetz |
| 264 | 1 | |c 19 Mar 1996 | |
| 300 | |a 22 | ||
| 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 29.09.2017 | ||
| 520 | |a We use gas-dynamical simulations of galaxy clusters to compare their X-ray and strong lensing properties. Special emphasis is laid on mass estimates. The cluster masses range between 6 x 10^14 solar masses and 4 x 10^15 solar masses, and they are examined at redshifts between 1 and 0. We compute the X-ray emission of the intracluster gas by thermal bremsstrahlung, add background contamination, and mimic imaging and spectral observations with current X-ray telescopes. Although the beta model routinely provides excellent fits to the X-ray emission profiles, the derived masses are typically biased low because of the restricted range of radii within which the fit can be done. For beta values of ~ 2/3, which is the average in our numerically simulated sample, the mass is typically underestimated by ~ 40 per cent. The masses of clusters which exhibit pronounced substructure are often substantially underestimated. We suggest that the ratio between peak temperature and emission-weighted average cluster temperature may provide a good indicator for ongoing merging and, therefore, for unreliable mass estimates. X-ray mass estimates are substantially improved if we fit a King density profile rather than the beta model to the X-ray emission, thereby dropping the degree of freedom associated with beta. Clusters selected for their strong lensing properties are typically dynamically more active than typical clusters. Bulk flows in the intracluster gas contain a larger than average fraction of the internal energy of the gas in such objects, hence the measured gas temperatures are biased low. The bulk of the optical depth for arc formation is contributed by clusters with intermediate rather than high X-ray luminosity. Arcs occur predominantly in clusters which exhibit substructure and are not in an equilibrium state. Finally we explain why the | ||
| 650 | 4 | |a Astrophysics | |
| 700 | 1 | |a Steinmetz, Matthias |d 1966- |e VerfasserIn |0 (DE-588)1014451787 |0 (DE-627)705236528 |0 (DE-576)348839391 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Arxiv |d Ithaca, NY : Cornell University, 1991 |g (1996) Artikel-Nummer 9603101, 22 Seiten |h Online-Ressource |w (DE-627)509006531 |w (DE-600)2225896-6 |w (DE-576)28130436X |7 nnas |a A comparison of X-ray and strong lensing properties of simulated X-ray clusters |
| 773 | 1 | 8 | |g year:1996 |g extent:22 |a A comparison of X-ray and strong lensing properties of simulated X-ray clusters |
| 856 | 4 | 0 | |u http://arxiv.org/abs/astro-ph/9603101 |x Verlag |z kostenfrei |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20170929 | ||
| 993 | |a Article | ||
| 998 | |g 141554185 |a Bartelmann, Matthias |m 141554185:Bartelmann, Matthias |p 1 |x j | ||
| 999 | |a KXP-PPN1563969157 |e 2982313669 | ||
| BIB | |a Y | ||
| JSO | |a {"id":{"eki":["1563969157"]},"name":{"displayForm":["Matthias Bartelmann and Matthias Steinmetz"]},"note":["Gesehen am 29.09.2017"],"type":{"bibl":"chapter","media":"Online-Ressource"},"language":["eng"],"title":[{"title":"A comparison of X-ray and strong lensing properties of simulated X-ray clusters","title_sort":"comparison of X-ray and strong lensing properties of simulated X-ray clusters"}],"relHost":[{"disp":"A comparison of X-ray and strong lensing properties of simulated X-ray clustersArxiv","physDesc":[{"extent":"Online-Ressource"}],"recId":"509006531","language":["eng"],"type":{"bibl":"edited-book","media":"Online-Ressource"},"note":["Gesehen am 28.05.2024"],"title":[{"title_sort":"Arxiv","title":"Arxiv"}],"origin":[{"publisher":"Cornell University ; Arxiv.org","dateIssuedDisp":"1991-","dateIssuedKey":"1991","publisherPlace":"Ithaca, NY ; [Erscheinungsort nicht ermittelbar]"}],"id":{"eki":["509006531"],"zdb":["2225896-6"]},"part":{"year":"1996","extent":"22","text":"(1996) Artikel-Nummer 9603101, 22 Seiten"},"titleAlt":[{"title":"Arxiv.org"},{"title":"Arxiv.org e-print archive"},{"title":"Arxiv e-print archive"},{"title":"De.arxiv.org"}],"pubHistory":["1991 -"]}],"person":[{"display":"Bartelmann, Matthias","given":"Matthias","role":"aut","family":"Bartelmann"},{"display":"Steinmetz, Matthias","role":"aut","given":"Matthias","family":"Steinmetz"}],"origin":[{"dateIssuedDisp":"19 Mar 1996","dateIssuedKey":"1996"}],"physDesc":[{"extent":"22 S."}],"recId":"1563969157"} | ||
| SRT | |a BARTELMANNCOMPARISON1919 | ||