The Molecular Cloud near the Hard X-Ray Source 1E 1740.7-2942

Details The Molecular Cloud near the Hard X-Ray Source 1E 1740.7-2942 The Molecular Cloud near the Hard X-Ray Source 1E 1740.7-2942

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...481..296y&link_type=abstract

Astrophysical Journal v.481, p.296

Astronomy and Astrophysics

Astronomy

17

Ism: Clouds, Ism: Molecules, Molecular Processes, Radiative Transfer, X-Rays: Stars

Scientific paper

We carry out calculations of the influence of the hard X-ray source 1E 1740.7-2942 on the dense molecular cloud in which it may be embedded. From the thermal, chemical, and ionization structure, we obtain the spatial distribution of the HCO+ 1--0 emission line. It matches the interferometric observations of the line well and supports the view of Phillips & Lazio that the source lies within the cloud near to its eastern edge. The intensity profiles of the 3--2 and 4--3 transitions of HCO+ are given. Their observation would provide further information on the location of the source. The abundances and spatial distribution of other molecular species are predicted.

Affiliated with

Also associated with

No associations

Rating

The Molecular Cloud near the Hard X-Ray Source 1E 1740.7-2942 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 The Molecular Cloud near the Hard X-Ray Source 1E 1740.7-2942, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Molecular Cloud near the Hard X-Ray Source 1E 1740.7-2942 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-836041