Photometric and spectral studies of pre-main-sequence stars

Details Photometric and spectral studies of pre-main-sequence stars Photometric and spectral studies of pre-main-sequence stars

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hell.confe.140s&link_type=abstract

"5th Hellenic Astronomical Conference, held 20-22 September, 2001 in Crete, Greece. Online at http://www.astro.auth.gr/elaset/he

Astronomy and Astrophysics

Astronomy

Scientific paper

In the pre-main-sequence stage of evolution the young stellar objects show different types of photometric variability. We report results from photometric and spectral observations in the regions of star formations: NGC 7129, NGC 7000 and Alpha Persei. Our investigations have for an object a long-term photometry of known pre-main sequence objects and discovery of new variable stars. The wide-field spectral studies ware used to reveal the new candidates for pre-main sequence objects. Using precise CCD photometric observations we try to determine their distribution on the spectrum-luminosity diagram.

Affiliated with

Also associated with

No associations

Rating

Photometric and spectral studies of pre-main-sequence stars 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 Photometric and spectral studies of pre-main-sequence stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric and spectral studies of pre-main-sequence stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1862970