dc.contributor.author |
Jeyakumar, S |
|
dc.contributor.author |
Stalin, C. S |
|
dc.contributor.author |
Coziol, R |
|
dc.date.accessioned |
2012-09-17T10:57:42Z |
|
dc.date.available |
2012-09-17T10:57:42Z |
|
dc.date.issued |
2011-10 |
|
dc.identifier.citation |
XIII Latin American Regional IAU Meeting,Morelia, Michoacán, México, November 8 - 12, 2010, edited by W. J. Henney & S. Torres-Peimbert, Rev. Mex. AA (Serie de Conferencias), Vol. 40, pp. 123 |
en |
dc.identifier.isbn |
978-607-02-2653-3 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/5905 |
|
dc.description |
Open Access |
en |
dc.description.abstract |
Light curves of the continuum at 5100 °A and
Hβ line are obtained from spectroscopic monitoring
observations of the Seyfert 1.5 galaxy
H 0507+164. The mass of the black hole is
calculated based on cross-correlation analysis
of these light curves. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Instituto de Astronomia, UNAM |
en |
dc.relation.uri |
http://www.astroscu.unam.mx/~rmaa/rmaa.html |
en |
dc.rights |
© Instituto de Astronomia, UNAM - XIII Latin American Regional IAU Meeting |
en |
dc.subject |
Galaxy |
en |
dc.subject |
Seyfert 1.5 Galaxy H 0507+164 |
en |
dc.subject |
Active Galactic Nuclei (AGNs) |
|
dc.title |
Reverberation mapping of the Seyfert 1.5 galaxy H 0507+164 |
en |
dc.type |
Article |
en |