Abstract
From PDS scans of the late-type spiral galaxies NGC 1313, 1365, 6946, and 7793, we determine the surface brightness distributions. These distributions enable us to calculate physical parameters such as Re*, μe, α-1D/B, C21, and M/L. The values of some of these parameters were also compiled from other studies, and all were compared with morphological type T. One of the meaningful results shows that there is a certain correlation between D/B and T, which is constant until T<-1 or 2, and then increases sharply for T>-1 or 2. This may support the validity of the intrinsic formation theory.
| Original language | English |
|---|---|
| Pages (from-to) | 195-197 |
| Number of pages | 3 |
| Journal | Astrophysics and Space Science |
| Volume | 119 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1986 Jan 1 |
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All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
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Correlation between the physical parameters and morphological type of spiral galaxies. / Kim, Sug Whan; Chun, Mun Suk.
In: Astrophysics and Space Science, Vol. 119, No. 1, 01.01.1986, p. 195-197.Research output: Contribution to journal › Article
TY - JOUR
T1 - Correlation between the physical parameters and morphological type of spiral galaxies
AU - Kim, Sug Whan
AU - Chun, Mun Suk
PY - 1986/1/1
Y1 - 1986/1/1
N2 - From PDS scans of the late-type spiral galaxies NGC 1313, 1365, 6946, and 7793, we determine the surface brightness distributions. These distributions enable us to calculate physical parameters such as Re*, μe, α-1D/B, C21, and M/L. The values of some of these parameters were also compiled from other studies, and all were compared with morphological type T. One of the meaningful results shows that there is a certain correlation between D/B and T, which is constant until T<-1 or 2, and then increases sharply for T>-1 or 2. This may support the validity of the intrinsic formation theory.
AB - From PDS scans of the late-type spiral galaxies NGC 1313, 1365, 6946, and 7793, we determine the surface brightness distributions. These distributions enable us to calculate physical parameters such as Re*, μe, α-1D/B, C21, and M/L. The values of some of these parameters were also compiled from other studies, and all were compared with morphological type T. One of the meaningful results shows that there is a certain correlation between D/B and T, which is constant until T<-1 or 2, and then increases sharply for T>-1 or 2. This may support the validity of the intrinsic formation theory.
UR - http://www.scopus.com/inward/record.url?scp=34250130163&partnerID=8YFLogxK
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U2 - 10.1007/BF00648845
DO - 10.1007/BF00648845
M3 - Article
AN - SCOPUS:34250130163
VL - 119
SP - 195
EP - 197
JO - Astrophysics and Space Science
JF - Astrophysics and Space Science
SN - 0004-640X
IS - 1
ER -