Results 311 to 320 of about 111,751 (340)

A comparison of the ingredients of stellar population models on the inference of the slope of the initial mass function.

, 2014
Chiara Spiniello, S. C. Trager
openalex   +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

Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]

Space Sci Rev
Szalay JR, Provornikova E, Ayari E, Bzowski M, Christian ER, Funsten HO, Galli A, Gkioulidou M, Horányi M, Livi S, McComas DJ, Möbius E, Ogasawara K, Rahmanifard F, Rankin JS, Reisenfeld DB, Schwadron NA, Sternovsky Z, Swaczyna P, Turner D, Zank GP, Zirnstein EJ.   +21 more
europepmc   +1 more source

Water Versus Land on Temperate Rocky Planets. [PDF]

Space Sci Rev
Guimond CM, Spohn T, Berdyugina S, Byrne PK, Coltice N, Glaser DM, Lingam M, Lineweaver CH, Cawood PA.   +8 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Origins of the Stellar Initial Mass Function

AIP Conference Proceedings, 2009
This paper gives a brief sketch of the current state of affairs in research into the origins of the stellar initial mass function. The likely origin of the IMF in the distribution of mass amongst dense cores in star forming regions is discussed, touching upon evidence from observations and predictions from theory.
Toby J. T. Moore, Giuliana Giobbi, Amedeo Tornambe, Gabriella Raimondo, Marco Limongi, L. A. Antonelli, Nicola Menci, Enzo Brocato   +7 more
openaire   +1 more source

Models of the Stellar Initial Mass Function

2014
In the past decade, we have witnessed a paradigm shift in star formation theory away from a quasi-static picture, where magnetic fields dominate the process, towards a much more dynamic and realistic approach. We now think that the process of stellar birth is controlled by the complex interplay between self-gravity and a number of opposing physical ...
Ralf S. Klessen, Simon C. O. Glover
openaire   +1 more source

Stellar mass functions of galaxies at 4

2014
23 pages, 18 figures.
Stefanon, Mauro, Marchesini, Danilo, Muzzin, Adam, Brammer, Gabriel G., Dunlop, James S., Franx, Marijin, Fynbo, Johan P. U., Labbe, Ivo, Milvang-Jensen, Bo, van Dokkum, Pieter G.   +9 more
openaire   +1 more source

The galaxy stellar mass function at 3.5

2014
The galaxy stellar mass function (GSMF) at high-z provides key information on star-formation history and mass assembly in the young Universe. We aimed to use the unique combination of deep optical/NIR/MIR imaging provided by HST, Spitzer and the VLT in the CANDELS-UDS, GOODS-South, and HUDF fields to determine the GSMF over the redshift range 3.54 ...
Grazian, A., Fontana, A., Santini, P., Dunlop, J. S., Ferguson, H. C., Castellano, M., Amorin, R., Ashby, M. L. N., Barro, G., Behroozi, P., Boutsia, K., Caputi, K. I., Chary, R. R., Dekel, A., Dickinson, M. A., Faber, S. M., Fazio, G. G., Finkelstein, S. L., Galametz, A., Giallongo, E., Giavalisco, M., Grogin, N. A., Guo, Y., Kocevski, D., Koekemoer, A. M., Koo, D. C., Lee, K. -S., Lu, Y., Merlin, E., Mobasher, B., Nonino, M., Papovich, C., Paris, D., Pentericci, L., Reddy, N., Renzini, A., Salmon, B., Salvato, M., Sommariva, V., Song, M., Vanzella, E.   +40 more
openaire   +1 more source

The Stellar Mass Function in Globular Clusters

2009
Globular clusters in our own Milky Way formed at redshift z≃5 or more, when the physical conditions of the environment, such as pressure, density, temperature and chemical composition, were very different from those found in current star forming regions.
openaire   +1 more source