ROSAT PSPC Observations of 27 Near--Main-Sequence B Stars

Details ROSAT PSPC Observations of 27 Near--Main-Sequence B Stars ROSAT PSPC Observations of 27 Near--Main-Sequence B Stars

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...487..867c&link_type=abstract

Astrophysical Journal v.487, p.867

Astronomy and Astrophysics

Astronomy

76

Radiation Mechanisms: Thermal, Shock Waves, Stars: Atmospheres, Stars: Early-Type, X-Rays: Stars

Scientific paper

In this paper, we report on ROSAT Position Sensitive Proportional Counter (PSPC) observations of 27 near--main-sequence B stars made with unprecedented sensitivity. Contrary to the results of previous surveys, it is found that 75% of the sample stars are X-ray sources, albeit most at modest levels. The X-ray luminosities of the program stars range from 5.6 x 1027 up to 2.2 x 1032 ergs s-1. We find that LX/LBol decreases abruptly beyond about B0 and stabilizes at LX/LBol ~ 10-8.5 by about B2, with seven nondetections at B2 and later. For the B0 and B1 stars, our modeling suggests that wind attenuation of the X-ray photons is significant, so that the emitted X-ray luminosity, corrected for this attenuation, actually exceeds 10-7LBol in some cases. Presumably, this situation is even more severe for O stars; thus, the well-known LX/LBol ~ 10-7 law simply may be an artifact of the neglect of wind attenuation. The ROSAT PSPC observations of most of the B stars are very soft, with the notable exception of tau Sco (B0 V). The wind emission measure filling factors that we find for the very early B stars are rather large (roughly 0.1--1). This could be brought into line with theoretical calculations of the line-force instability, wind-shock mechanism if the mass-loss rates of these stars are a few times higher than theory currently predicts. However, the X-rays from stars later than B2 require filling factors greater than unity and thus cannot be produced by any radiation-driven wind-shock mechanism because there is simply not enough wind material to produce the observed X-rays. It is possible that mid- to late-B stars represent some kind of transition to, or hybrid of, wind and coronal X-ray mechanisms.

Affiliated with

Also associated with

No associations

Rating

ROSAT PSPC Observations of 27 Near--Main-Sequence B Stars 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 ROSAT PSPC Observations of 27 Near--Main-Sequence B Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ROSAT PSPC Observations of 27 Near--Main-Sequence B Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1769191