Spectroscopy and BVI photometry of the young open cluster NGC 6604
arXiv:astro-ph/0004012 · doi:10.1051/aas:2000193
Abstract
BVI photometry (from South Africa Astron. Obs.), Echelle high resolution spectroscopy and AFOSC integral field spectroscopy (from Asiago, Italy) of the young open cluster NGC 6604 are presented. Age, distance, reddening, membership, radial and rotational velocities are derived and discussed. An age of 5 million years, a distance of 1.7 kpc and a reddening E(B-V)=1.02 are found. The cluster radial velocity is in agreement with the Hron (1987) model for the Galaxy disk rotation. Pre-ZAMS objects are not present down to M_V = +1.5 mag.
arXiv commentaccepted in Astron.Astrophys.Suppl. Figure 2 is degraded in resolution
Cited by in corpus (9)
- Massive stars exploding in a He-rich circumstellar medium. I. Type Ibn (SN 2006jc-like) events
- The Evolutionary Status of Be Stars: Results from a Photometric Study of Southern Open Clusters
- The circumstellar environment and evolutionary state of the supergiant B[e] star Wd1-9
- Optical Photometry of Type II-P Supernova 2004dj in NGC 2403
- Quasi-simultaneous XMM-Newton and VLA observation of the non-thermal radio emitter HD\168112 (O5.5III(f^+))
- An XMM-Newton observation of the multiple system HD167971 (O5-8V + O5-8V + (O8I)) and the young open cluster NGC6604
- MY Serpentis: a high-mass triple system in the Ser OB2 association
- Mass segregation in diverse environments
- Survey of Profile Parameters of the Diffuse Interstellar Band. From Uniform Profiles to Doppler Splitting and Blueshifts