Hydra Archive [Hectospec Public Archive] [SAO/TDC Public Archive]

Program Code	HXP
Program Name	Accretion Signatures and Cluster Membership in h & chi Persei
Principal Investigator	Thayne Currie [email]  [web]
Co-Investigators	Scott Kenyon, Nancy Evans
Abstract	These Hydra observations of pre-main sequence stars in h and chi Persei cover approximately 0.5 square degrees on the sky, encompassing the h and chi Persei star-forming region. From this program we will better constrain the initial mass function and cluster membership down to solar masses. We will also search for evidence of gas accretion from the H alpha line widths. We shall use such data to better constrain the timescale for gas accretion onto protostars as well as investigate any dependence that the gas accretion timescale might have on the stellar environment and properties of the central star.
Spectra	[search in archive]
Semesters data was taken	2000B, 2001B
Papers	none
Other links	Hectospec Public Data for this program FAST Public Data for this program

[Hydra Spectrograph] [Hectospec Public Data] [FAST Public Data] [SAO/TDC Archived Data]

Last modified on
Comments or Questions? Contact the TDC Archive Group