Proxima Cen chromospheric emission lines (Fuhrmeister+, 2011)

Details Proxima Cen chromospheric emission lines (Fuhrmeister+, 2011) Proxima Cen chromospheric emission lines (Fuhrmeister+, 2011)

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35349133f&link_type=abstract

VizieR On-line Data Catalog: J/A+A/534/A133. Originally published in: 2011A&A...534A.133F

Physics

Stars: Variable, Stars: Late-Type, Spectroscopy

Scientific paper

We present an extensive identification catalog of chromospheric emission lines in the optical range for a flare on Proxima Centauri. The data were obtained with ESO's Kueyen telescope equipped with the UVES spectrograph on March 9/10, 11/12, 13/14 in 2009. The instrument was operated in dichroic mode (spectral coverage from 3290 to 4500 and from 6400 to 10080Å). We tabulate measured wavelength, line flux and FWHM for every line and also provide the rest wavelength from the Moore catalog which was used for identification (Moore, 1972, Nat. Stand. Ref. Data. Ser., 40). Few lines were identified with the NIST database.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Proxima Cen chromospheric emission lines (Fuhrmeister+, 2011) 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 Proxima Cen chromospheric emission lines (Fuhrmeister+, 2011), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Proxima Cen chromospheric emission lines (Fuhrmeister+, 2011) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1671551