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Bastian, N., Konstantopoulos, I. S., Trancho, G., Weisz, D. R., Larsen, S. S., Fouesneau, M., Kaschinski, C. B., Gieles, M. (2012) Spectroscopic constraints on the form of the stellar cluster mass function. Astronomy & Astrophysics, 541. doi:10.1051/0004-6361/201219079

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Reference TypeJournal (article/letter/editorial)
TitleSpectroscopic constraints on the form of the stellar cluster mass function
JournalAstronomy & Astrophysics
AuthorsBastian, N.Author
Konstantopoulos, I. S.Author
Trancho, G.Author
Weisz, D. R.Author
Larsen, S. S.Author
Fouesneau, M.Author
Kaschinski, C. B.Author
Gieles, M.Author
Year2012 (May)Volume541
PublisherEDP Sciences
DOIdoi:10.1051/0004-6361/201219079Search in ResearchGate
Generate Citation Formats
Mindat Ref. ID3476901Long-form Identifiermindat:1:5:3476901:4
GUID0
Full ReferenceBastian, N., Konstantopoulos, I. S., Trancho, G., Weisz, D. R., Larsen, S. S., Fouesneau, M., Kaschinski, C. B., Gieles, M. (2012) Spectroscopic constraints on the form of the stellar cluster mass function. Astronomy & Astrophysics, 541. doi:10.1051/0004-6361/201219079
Plain TextBastian, N., Konstantopoulos, I. S., Trancho, G., Weisz, D. R., Larsen, S. S., Fouesneau, M., Kaschinski, C. B., Gieles, M. (2012) Spectroscopic constraints on the form of the stellar cluster mass function. Astronomy & Astrophysics, 541. doi:10.1051/0004-6361/201219079
In(2012) Astronomy & Astrophysics Vol. 541. EDP Sciences

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Gieles, M., Larsen, S. S., Scheepmaker, R. A., Bastian, N., Haas, M. R., Lamers, H. J. G. L. M. (2006) Observational evidence for a truncation of the star cluster initial mass function at the high mass end. Astronomy & Astrophysics, 446 (2). doi:10.1051/0004-6361:200500224
Gieles, M., Larsen, S. S., Bastian, N., Stein, I. T. (2006) The luminosity function of young star clusters: implications for the maximum mass and luminosity of clusters. Astronomy & Astrophysics, 450 (1). 129-145 doi:10.1051/0004-6361:20053589
Konstantopoulos, I. S., Bastian, N., Smith, L. J., Westmoquette, M. S., Trancho, G., Gallagher, J. S. (2009) A SPECTROSCOPIC CENSUS OF THE M82 STELLAR CLUSTER POPULATION,. The Astrophysical Journal, 701 (2). 1015-1031 doi:10.1088/0004-637x/701/2/1015
Scheepmaker, R. A., Haas, M. R., Gieles, M., Bastian, N., Larsen, S. S., Lamers, H. J. G. L. M. (2007) ACSimaging of star clusters in M 51. Astronomy & Astrophysics, 469 (3). 925-940 doi:10.1051/0004-6361:20077511
Bastian, N., Adamo, A., Gieles, M., Lamers, H. J. G. L. M., Larsen, S. S., Silva-Villa, E., Smith, L. J., Kotulla, R., Konstantopoulos, I. S., Trancho, G., Zackrisson, E. (2011) Evidence for environmentally dependent cluster disruption in M83. Monthly Notices of the Royal Astronomical Society: Letters, 417. doi:10.1111/j.1745-3933.2011.01103.x
Smith, L. J., Bastian, N., Konstantopoulos, I. S., Gallagher III, J. S., Gieles, M., de Grijs, R., Larsen, S. S., O'Connell, R. W., Westmoquette, M. S. (2007) The Young Cluster Population of M82 Region B. The Astrophysical Journal, 667 (2). doi:10.1086/522120
Evans, C. J., Castro, N., Gonzalez, O. A., Garcia, M., Bastian, N., Cioni, M.-R. L., Clark, J. S., Davies, B., Ferguson, A. M. N., Kamann, S., Lennon, D. J., Patrick, L. R., Vink, J. S., Weisz, D. R. (2019) First stellar spectroscopy in Leo P. Astronomy & Astrophysics, 622. doi:10.1051/0004-6361/201834145
Konstantopoulos, I. S., Bastian, N., Smith, L. J., Trancho, G., Westmoquette, M. S., Gallagher III, J. S. (2008) Gemini Spectroscopy andHSTImaging of the Stellar Cluster Population in Region B of M82. The Astrophysical Journal, 674 (2). 846-856 doi:10.1086/524133
Eitner, P., Bergemann, M., Hansen, C. J., Cescutti, G., Seitenzahl, I. R., Larsen, S., Plez, B. (2020) Observational constraints on the origin of the elements. Astronomy & Astrophysics, 635. doi:10.1051/0004-6361/201936603
Gieles, M., Bastian, N., Lamers, H. J. G. L. M., Mout, J. N. (2005) The star cluster population of M 51. Astronomy & Astrophysics, 441 (3). 949-960 doi:10.1051/0004-6361:20052914
Bastian, N., Gieles, M., Lamers, H. J. G. L. M., Scheepmaker, R. A., de Grijs, R. (2005) The star cluster population of M 51. Astronomy & Astrophysics, 431 (3). 905-924 doi:10.1051/0004-6361:20041078
 
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