نتائج البحث - "R M Rich"

المساهمون: Ferraro, F. R., Pallanca, C., Lanzoni, B., Crociati, C., Dalessandro, E., Origlia, L., Rich, R. M., Saracino, S., Mucciarelli, A., Valenti, E., Geisler, D., Mauro, F., Villanova, S., Moni Bidin, C., Beccari, G.

المصدر: Nature Astronomy. 5:311-318

وصف الملف: STAMPA

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ca7f8529cb14de7908697969cbb2c3f
https://doi.org/10.1038/s41550-020-01267-y

Find this article in full text from Springer Verlag.

Find this article in full text from ProQuest

9

First r-process enhanced star confirmed as a member of the Galactic bulge

المؤلفون: R. Forsberg, R. M. Rich, N. Nieuwmunster, H. Jönsson, M. Schultheis, N. Ryde, B. Thorsbro

المصدر: Astronomy & Astrophysics. 669:A17

مصطلحات موضوعية: Space and Planetary Science, Astronomy and Astrophysics

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_________::61f986c8a4e7da5eab1db69145a6406b
https://doi.org/10.1051/0004-6361/202244305

10

Evidence for Cold-stream to Hot-accretion Transition as Traced by Ly{\alpha} Emission from Groups and Clusters at 2 < z < 3.3

المؤلفون: E. Daddi, R. M. Rich, F. Valentino, S. Jin, I. Delvecchio, D. Liu, V. Strazzullo, J. Neill, R. Gobat, A. Finoguenov, F. Bournaud, D. Elbaz, B. S. Kalita, D. O’Sullivan, T. Wang

المساهمون: Department of Physics, Doctoral Programme in Particle Physics and Universe Sciences, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay

المصدر: Daddi, E, Rich, R M, Valentino, F, Jin, S, Delvecchio, I, Liu, D, Strazzullo, V, Neill, J, Gobat, R, Finoguenov, A, Bournaud, F, Elbaz, D, Kalita, B S, O’Sullivan, D & Wang, T 2022, ' Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3 ', The Astrophysical Journal Letters, vol. 926, no. 2, L21 . https://doi.org/10.3847/2041-8213/ac531f
Daddi, E, Rich, R M, Valentino, F, Jin, S, Delvecchio, I, Liu, D, Strazzullo, V, Neill, J, Gobat, R, Finoguenov, A, Bournaud, F, Elbaz, D, Kalita, B S, O'Sullivan, D & Wang, T 2022, ' Evidence for Cold-stream to Hot-accretion Transition as Traced by Ly α Emission from Groups and Clusters at 2 < z < 3.3 ', Astrophysical Journal Letters, vol. 926, no. 2, L21 . https://doi.org/10.3847/2041-8213/ac531f
Astrophys.J.Lett.
Astrophys.J.Lett., 2022, 926 (2), pp.L21. ⟨10.3847/2041-8213/ac531f⟩

مصطلحات موضوعية: Cosmology and Nongalactic Astrophysics (astro-ph.CO), IMPACT, Astrophysics::High Energy Astrophysical Phenomena, REDSHIFT, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxy accretion, 115 Astronomy, Space science, 114 Physical sciences, Astrophysics - Astrophysics of Galaxies, SHOCKS, QUASARS, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Galaxy evolution, LUMINOSITY, Astrophysics::Solar and Stellar Astrophysics, GALAXY FORMATION, Astrophysics::Earth and Planetary Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], BLOBS, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics

وصف الملف: application/pdf

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a77ef2658ac36a09ed28b3f832f710c4
http://arxiv.org/abs/2202.03715

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