Abstract
We present new counts of stars in M15, using plates in B, V and U. We are able to explore relatively close to the central parts of the cluster (0.1 pc) and we derive the best fitting parameters for the star distribution.
Calvani, M;
[1]
Nobili, L;
[2]
Turolla, R
[3]
- Padua Univ. (Italy). Ist. di Astronomia
- Padua Univ. (Italy). Ist. di Fisica
- Scuola Internazionale Superiore di Studi Avanzati, Trieste (Italy)
Citation Formats
Calvani, M, Nobili, L, and Turolla, R.
Star counts in M15 on U, B and V plates.
Netherlands: N. p.,
1980.
Web.
doi:10.1007/BF00642373.
Calvani, M, Nobili, L, & Turolla, R.
Star counts in M15 on U, B and V plates.
Netherlands.
https://doi.org/10.1007/BF00642373
Calvani, M, Nobili, L, and Turolla, R.
1980.
"Star counts in M15 on U, B and V plates."
Netherlands.
https://doi.org/10.1007/BF00642373.
@misc{etde_6140169,
title = {Star counts in M15 on U, B and V plates}
author = {Calvani, M, Nobili, L, and Turolla, R}
abstractNote = {We present new counts of stars in M15, using plates in B, V and U. We are able to explore relatively close to the central parts of the cluster (0.1 pc) and we derive the best fitting parameters for the star distribution.}
doi = {10.1007/BF00642373}
journal = []
volume = {73:1}
journal type = {AC}
place = {Netherlands}
year = {1980}
month = {Nov}
}
title = {Star counts in M15 on U, B and V plates}
author = {Calvani, M, Nobili, L, and Turolla, R}
abstractNote = {We present new counts of stars in M15, using plates in B, V and U. We are able to explore relatively close to the central parts of the cluster (0.1 pc) and we derive the best fitting parameters for the star distribution.}
doi = {10.1007/BF00642373}
journal = []
volume = {73:1}
journal type = {AC}
place = {Netherlands}
year = {1980}
month = {Nov}
}