Recensie: The Dibs – Just For You ★★★★
https://writteninmusic.com/albumrecensie/the-dibs-just-for-you/
“Soul Food” staat er in vette letters gekalkt in de cd-houder en dat debiteren The Dibs, een Belgisch /Nederlands bluescombo aangevoerd door Peter Jacobs. De allereerste keer zag ik Peter Jacobs in de vroege jaren negentig op een podium met Marc Thijs, nog voor The Electric Kings en TEE periode, met The Healers op Grenslandblues, […]
Estes são sobras da última campanha mesmo por isso se algum fediamigo quiser é melhor mandar #dibs já (metendo 5€ no https://ppl.pt/sarilho4)
Tem:
🔹 Porta-chaves Ângela fofa em acrílico translúcido
🔹 Pin dourado da Infantaria do MAI
🔹 Fita-cola de papel do Gabinete do Augúrio
Yurt dışında yerleşiklerin hisse senedi, DİBS ve ÖST stoku!: urt dışında yerleşik kişiler, geçen hafta 93,2 milyon dolarlık hisse senedi aldı.
Türkiye Cumhuriyet Merkez Bankası (TCMB) tarafından "Haftalık Menkul Kıymet İstatistikleri" yayımlandı.
Buna göre yurt dışında yerleşik kişiler, 30 Mayıs haftasında net 93,2 milyon dolarlık hisse senedi alırken, 333,5 milyon dolarlık Devlet İç Borçlanma Senedi (DİBS) ve… https://www.eshahaber.com.tr/haber/yurt-disinda-yerlesiklerin-hisse-senedi-dibs-ve-ost-stoku-231030.html?utm_source=dlvr.it&utm_medium=mastodon EshaHaber.com.tr #hisse #ekonomi #DİBS #ÖST #yurt
[ABRIDGED] DIBs are faint absorption features of mainly unknown origin. Observational constraints on their carriers have been provided in the vast majority of the cases via observations in our Galaxy. Detections in other galaxies are scarce. However, they can further constrain the nature of the carriers by sampling different environments and they can put into test the ubiquity of the molecules creating these features. Using the MUSE data of the LIRG NGC 6240, we mapped the DIB5780 over an almost contiguous area of ~76.96 kpc^2 in the center of the system. We also traced the DIBl6284 over two separate areas toward the north and south of the system, with an extent of ~21.22 kpc^2 and ~31.41 kpc^2 (with a total detected area of ~59.78 kpc^2). This is the first time that the l6284 DIB has been mapped outside our Galaxy. Both maps were compared with the attenuation on the overall stellar population and the ionised gas. Both DIBs are detected in locations with high attenuation (E(B-V)_Gas} > 0.3 and E(B-V)_Stellar >0.1), supporting the connection between DIB carriers and dust. Moreover, when compared with other galaxies, DIBs correlate better with stellar than with the ionised gas attenuation. The DIBl6284 presents a stronger correlation with reddening than the l5780 DIB does that can be attributed to a different nature of the carriers causing these DIBs, or a combined effect of a dependency with the metallicity and the different locations where these DIBs have been measured. In addition, we show that NaI D strongly correlates with both DIBs and advocate the usage of DIBs as a first order tracer for amount of material, in the case where NaI D reaches saturation. The findings here show that DIB carriers can exist and survive in an environment as extreme as a galaxy hosting AGN and allow to envision the possibilities integral field spectrographs have to study DIBs well beyond our Galaxy.
Written in Music
Loren Kohnfelder
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The Book (2nd Edition)
Shizamura está recuperando 🌟
EshaHaber
Pᵉtɘr Wᵉil8acher
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