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33 results on '"Stars: mass function"'

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1. Constraints on the stellar upper mass limit from simulations of UV disk ablation.

2. Constraints on the stellar upper mass limit from simulations of UV disk ablation.

3. Correction to 'The impact of carbon and oxygen abundances on the metal-poor initial mass function'.

4. Radial variation of the stellar mass functions in the globular clusters M15 and M30: clues of a non-standard IMF?

5. Analyse spectro-photométrique des naines blanches froides dans l'échantillon Gaia

7. On the Mass Distribution of Stellar-Mass Black Holes

8. The IMF in the Galactic Disk and Bulge are Indistinguishable.

9. The Young and the Massive: Stars at the upper end of the Initial Mass Function.

10. From the CMF to the IMF: Beyond the core-collapse model

11. From the CMF to the IMF: Beyond the core-collapse model

12. Our Nearest 15 Million Neighbors: The Field Low—Mass Stellar Luminosity and Mass Functions.

13. The initial mass function in clusters: theoretical and observational perspectives.

14. Sampling effects in the emission-line spectra of Hii regions.

15. Galactic archeology with extremely metal-poor stars.

16. Young Star Clusters in the Small Magellanic Cloud: Impact of Local and Global Conditions on Star Formation.

17. Modelling the evolution and nucleosynthesis of carbon-enhanced metal-poor stars.

18. Clump lifetimes and the initial mass function.

19. The position angle of the Galactic bulge.

20. Molecular clouds in galaxies as seen from NIR extinction studies.

21. On the Mass Distribution of Stellar-Mass Black Holes

22. Hα and FUV luminosities from a stochastically formed stellar population.

23. Young Star Clusters in the Small Magellanic Cloud: Impact of Local and Global Conditions on Star Formation

24. The puzzling frequencies of CEMP and NEMP stars

25. Modelling the evolution and nucleosynthesis of carbon-enhanced metal-poor stars

26. The importance of initial conditions and metallicity for the fragmentation of protogalactic gas.

27. Observations of clusters with ages from 0.01 to 1.0 Gyr in the Large Magellanic Cloud.

28. N-body Simulations of Star Clusters.

30. Sampling effects in the emission line spectra of HII regions.

31. N -body Simulations of Star Clusters.

32. Empirical evidence suggesting a stellar upper-mass limit.

33. The dependence of the IMF on the density- temperature relation of pre-stellar gas.

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