Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..729....1s&link_type=abstract
The Astronomer's Telegram, #729
Astronomy and Astrophysics
Astronomy
Radio, Novae, Supernovae
Scientific paper
We report the lack of detection of radio emission near the position of the type-Ia supernova 2006X (IAUC 8667, CBET 393) with the Very Large Array: Upper limits (3 sigma) to any radio flux density were established on 2006 Feb. 09.37 UT of <0.162 mJy (Spectral Luminosity < 5.6 x 10^25 erg/s/Hz) at 22.460 GHz (wavelength 1.3 cm) and <0.047 mJy (Spectral Luminosity < 1.5 x 10^25 erg/s/Hz) at 8.460 GHz (wavelength 3.5 cm), among the deepest and earliest limits yet obtained for radio emission from a type Ia supernova.
Immler Stefan
Kelley Michael
Panagia Nino
Sramek Richard A.
Stockdale Christopher John
No associations
LandOfFree
Supernova 2006X in NGC 4321 (M100) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Supernova 2006X in NGC 4321 (M100), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernova 2006X in NGC 4321 (M100) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1766796