Optical Photometry of the New Optical Transient SN 2010da in NGC 300

Details Optical Photometry of the New Optical Transient SN 2010da in NGC 300 Optical Photometry of the New Optical Transient SN 2010da in NGC 300

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2640....1b&link_type=abstract

The Astronomer's Telegram, #2640

Astronomy and Astrophysics

Astronomy

4

Optical, Novae, Supernovae, Transients, Variables

Scientific paper

Multicolor images of the new optical transient in NGC 300, discovered by B. Monard (CBET #2289 and private communication), were obtained on 2010 May 25.37 by J. Espinoza with the SMARTS 1.3m telescope at Cerro Tololo and the ANDICAM camera. The transient has received the designation SN 2010da, although spectroscopic observations and the low luminosity suggest that it is most probably an LBV-like outburst on a dust-enshrouded massive star and not a true supernova (e.g., ATEL #2632, #2633, #2636, #2637, #2638).

Affiliated with

Also associated with

No associations

Rating

Optical Photometry of the New Optical Transient SN 2010da in NGC 300 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 Optical Photometry of the New Optical Transient SN 2010da in NGC 300, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical Photometry of the New Optical Transient SN 2010da in NGC 300 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-915122