Results 261 to 270 of about 239,171 (281)

Cosmology and fundamental physics with the ELT-ANDES spectrograph. [PDF]

Exp Astron (Dordr)
Martins CJAP, Cooke R, Liske J, Murphy MT, Noterdaeme P, Schmidt TM, Alcaniz JS, Alves CS, Balashev S, Cristiani S, Di Marcantonio P, Génova Santos R, Gonçalves RS, González Hernández JI, Maiolino R, Marconi A, Marques CMJ, Melo E Sousa MAF, Nunes NJ, Origlia L, Péroux C, Vinzl S, Zanutta A.   +22 more
europepmc   +1 more source

Identification of a turnover in the initial mass function of a young stellar cluster down to 0.5 MJ

De Furio M, Meyer M, Greene T, Hodapp K, Johnstone D, Leisenring J, Rieke M, Robberto M, Roellig T, Cugno G, Fiorellino E, Manara C, Raileanu R, Terwisga Sv.   +13 more
europepmc   +1 more source

High-temperature ²⁰⁵Tl decay clarifies ²⁰⁵Pb dating in early Solar System. [PDF]

Nature
Leckenby G, Sidhu RS, Chen RJ, Mancino R, Szányi B, Bai M, Battino U, Blaum K, Brandau C, Cristallo S, Dickel T, Dillmann I, Dmytriiev D, Faestermann T, Forstner O, Franczak B, Geissel H, Gernhäuser R, Glorius J, Griffin C, Gumberidze A, Haettner E, Hillenbrand PM, Karakas A, Kaur T, Korten W, Kozhuharov C, Kuzminchuk N, Langanke K, Litvinov S, Litvinov YA, Lugaro M, Martínez-Pinedo G, Menz E, Meyer B, Morgenroth T, Neff T, Nociforo C, Petridis N, Pignatari M, Popp U, Purushothaman S, Reifarth R, Sanjari S, Scheidenberger C, Spillmann U, Steck M, Stöhlker T, Tanaka YK, Trassinelli M, Trotsenko S, Varga L, Vescovi D, Wang M, Weick H, Yagüe Lopéz A, Yamaguchi T, Zhang Y, Zhao J.   +58 more
europepmc   +1 more source

On the Expansion of the Orion-Nebula Cluster

The Astrophysical Journal, 1971
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A new star in the nebula of Orion

The Astronomical Journal, 1897
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Variations in the spectrum of the Orion nebula.

The Astrophysical Journal, 1897
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The Distance of the Orion Nebula [PDF]

Publications of the Astronomical Society of the Pacific, 1931
The fainter stars situated in the central part of the Orion nebula, in the immediate neighborhood of the Trapezium, form a well-marked cluster quite comparable with other galactic star clusters ; for convenience we may call it the Trapezium cluster. This cluster is not well shown on ordinary photographs on account of the great brightness of the nebula ...
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The structure of the Orion nebula

Publications of the Astronomical Society of the Pacific, 1974
The Orion nebula is the best studied of all H II regions. The experimental data for this nebula are reviewed, and interpretive models of the structure of both the nebula and its environs are developed. The H II region is composed of an inner 3-min core surrounding the exciting star theta 1 C which is partially imbedded on the near side of a massive ...
R. H. Gammon, R. M. Hjellming, B. Balick
openaire   +2 more sources