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http://hdl.handle.net/2289/1904
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DC Field | Value | Language |
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dc.contributor.author | Pandey, S.B. | - |
dc.contributor.author | Anupama, G.C. | - |
dc.contributor.author | Sagar, R. | - |
dc.contributor.author | Bhattacharya, D. | - |
dc.contributor.author | Sahu, D.K. | - |
dc.contributor.author | Pandey, J.C. | - |
dc.date.accessioned | 2007-01-23T11:23:02Z | - |
dc.date.available | 2007-01-23T11:23:02Z | - |
dc.date.issued | 2003-04 | - |
dc.identifier.citation | Monthly Notice of the Royal Astronomical Society, 2003, Vol.340, p375-380 | en |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.uri | http://hdl.handle.net/2289/1904 | - |
dc.description | Restricted Access. An open access version is available at NASA ADS (alternative location). | en |
dc.description.abstract | We present the UBVRcIc broad-band optical photometry of the Type Ic supernova SN 2002ap obtained during 2002 February 6-March 23 in the early decline phases and also later on 2002 August 15. Combining these data with the published ones, the general light-curve development is studied. The time and luminosity of the peak brightness and the peak width are estimated. There is a flattening in the optical light curve about 30 d after the B maximum. The flux decline rates before flattening are 0.127 +/- 0.005, 0.082 +/- 0.001, 0.074 +/- 0.001, 0.062 +/- 0.001 and 0.040 +/- 0.001 mag d-1 in U, B, V, Rc and Ic passbands respectively, while the corresponding values after flattening are about 0.02 mag d-1 in all the passbands. The maximum brightness of SN 2002ap, MV=-17.2 mag, is comparable to that of the type Ic 1997ef, but fainter than that of the type Ic hypernova SN 1998bw. The peak luminosity indicates an ejection of ~0.06 Msolar56Ni mass. We also present low-resolution optical spectra obtained during the early phases. The SiII absorption minimum indicates that the photospheric velocity decreased from ~21 360 km s-1 to ~10 740 km s-1 during a period of ~6 d. | en |
dc.format.extent | 8338 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Blackwell Publishing for the Royal Astronomical Society | en |
dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?2003MNRAS.340..375P | en |
dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003MNRAS.340..375P&link_type=ARTICLE&db_key=AST | en |
dc.rights | (2003) Royal Astronomical Society | en |
dc.subject | techniques: photometric | en |
dc.subject | techniques: spectroscopic | en |
dc.subject | supernovae: general | en |
dc.title | A flattening in the optical light curve of SN 2002ap | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2003 MNRAS V340 p375.pdf Restricted Access | Restricted Access | 187.43 kB | Adobe PDF | View/Open Request a copy |
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