Ruprecht 55: an OB association at the edge of our Galaxy

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Stars: Early-Type, Ism: Bubbles, Ism: Kinematics And Dynamics, Open Clusters And Associations: Individual: Ruprecht 55, Galaxy: Structure

Scientific paper

We present new spectroscopy in the optical range and 21-cm HI data covering the Ruprecht 55 (Ru 55) field in the Puppis window where several authors have proposed the existence of one (or two) clusters.
We have determined new MK spectral types for about 50 stars in the region, finding 43 OB-type stars among them. LS 985 was found to be an O9 V + O9.5 III binary and it is the earliest type of star in our observed sample.
We have identified a stellar OB association (Ru 55), which is most likely related to a depletion detected in our HI data, as: (i) they are located at the same distance (6 kpc), within observational errors; (ii) both have similar radial velocities (~67 km s-1) (iii) current OB stars could have provided the energy needed to blow the cavity; (iv) the dynamical time-scale for the hole buildup matches the age estimated for the earliest OB stars; and (v) LS 985 might be responsible for ionizing the HI cavity inner walls close to it.

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

Ruprecht 55: an OB association at the edge of our Galaxy 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 Ruprecht 55: an OB association at the edge of our Galaxy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ruprecht 55: an OB association at the edge of our Galaxy will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1464354

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