Episode 13 - Missing Europium, Pluto's craters, 43,000 Goblins and some Pop III stars
カートのアイテムが多すぎます
カートに追加できませんでした。
ウィッシュリストに追加できませんでした。
ほしい物リストの削除に失敗しました。
ポッドキャストのフォローに失敗しました
ポッドキャストのフォロー解除に失敗しました
Episode 13 - Missing Europium, Pluto's craters, 43,000 Goblins and some Pop III stars
-
ナレーター：
-
著者：
このコンテンツについて
In this episode, Michelle and Payel discuss why dark matter halos have a Universal density profile, how to age-date Pluto's surface with craters, delayed Pop III star formation, dwarf candidates in the UNIONS survey, a problem with Europium and whether Little Red Dots are really AGN. Listen below, on Spotify, Apple podcasts or wherever you get your podcasts!
Read this episodes papers through the links below!
Collisionless relaxation to quasi-steady state attractors in cold dark matter halos: origin of the universal NFW profile - Uddipan Banik, Amitava Bhattacharjee
Pluto Geologic Map: Use of Crater Data to Understand Age Relationships - Kelsi N. Singer et al.
Bursty or heavy? The surprise of bright Population III systems in the Reionization era - Alessandra Venditti et al.
Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey - Nick Heesters et al.
Europium, we have a problem. Modelling r-process enrichment across Local Group galaxies - Marco Palla et al.
Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions - María de las Mercedes Carranza Escudero