Star formation in the large globule L810

Details Star formation in the large globule L810 Star formation in the large globule L810

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...153..253n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 153, no. 1, Dec. 1985, p. 253-259.

Astronomy and Astrophysics

Astrophysics

31

Globular Clusters, Nebulae, Star Formation, Water Masers, H Alpha Line, Infrared Spectra, Radio Observation, Stellar Luminosity

Scientific paper

The authors report on observations of the globule L 810, ranging from optical to radio wavelengths. The radio data suggest a kinematic distance of 1.5±0.5 kpc. The cloud mass is about 500 M_sun; and the total luminosity 350 L_sun;. At the position of the NH3 peak a near infrared source was found, which seems to be the dominant heating source of the cloud. A narrow filament emanating from this source shows Hα and the [S II] lines 6717 Å, 6731 Å. In the direction of the filament a nearby H2O maser was found. L 810 is the first isolated globule where a recently formed intermediate mass star associated with an H2O maser has been observed.

Affiliated with

Also associated with

No associations

Rating

Star formation in the large globule L810 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 Star formation in the large globule L810, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star formation in the large globule L810 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1159375