SDSSJ150634.27+013331.6: the second compact elliptical galaxy in the NGC5846 group

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5 pages, 4 figure, 1 table. Accepted to MNRAS Letters

Scientific paper

We report the discovery of the second compact elliptical (cE) galaxy SDSSJ150634.27+013331.6 in the nearby NGC5846 group by the Virtual Observatory (VO) workflow . This object (M_B = -15.98 mag, R_e = 0.24 kpc) becomes the fifth cE where the spatially-resolved kinematics and stellar populations can be obtained. We used archival HST WFPC2 images to demonstrate that its light profile has a two-component structure, and integrated photometry from GALEX, SDSS, UKIDSS, and Spitzer to build the multi-wavelength SED to constraint the star formation history (SFH). We observed this galaxy with the PMAS IFU spectrograph at the Calar-Alto 3.5m telescope and obtained two-dimensional maps of its kinematics and stellar population properties using the full-spectral fitting technique. Its structural, dynamical and stellar population properties suggest that it had a massive progenitor heavily tidally stripped by NGC5846.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

SDSSJ150634.27+013331.6: the second compact elliptical galaxy in the NGC5846 group 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 SDSSJ150634.27+013331.6: the second compact elliptical galaxy in the NGC5846 group, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SDSSJ150634.27+013331.6: the second compact elliptical galaxy in the NGC5846 group will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-677726

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.