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Evidence for Extremely High Dust Polarization Efficiency in NGC 3184
Recent studies have found the Type II-plateau supernova (SN) 1999gi tobe highly polarized (pmax=5.8%, where pmax is thehighest degree of polarization measured in the optical bandpass) andminimally reddened [E(B-V)=0.21+/-0.09 mag]. From multiple lines ofevidence, including the convincing fit of a ``Serkowski'' interstellarpolarization (ISP) curve to the continuum polarization shape, weconclude that the bulk of the observed polarization is likely due todust along the line of sight and is not intrinsic to SN 1999gi. Wepresent new spectropolarimetric observations of four distant Galacticstars close to the line of sight to SN 1999gi (two are within 0.02d) andfind that all are null to within 0.2%, effectively eliminating Galacticdust as the cause of the high polarization. The high ISP coupled withthe low reddening implies an extraordinarily high polarizationefficiency for the dust along this line of sight in NGC 3184:ISP/E(B-V)=31+22-9% mag -1. This isinconsistent with the empirical Galactic limit [ISP/E(B-V)<9%mag-1] and represents the highest polarization efficiency yetconfirmed for a single sight line in either the Milky Way or an externalgalaxy.
| Magnetic fields around BOK globules: CCD polarimetry of CB 4
The small Bok globule CB 4 was probed using a CCD imaging polarimeter inorder to create a detailed map of the magnetic field associated withthis cloud. Stars as faint as 17th mag at V band were measuredpolarimetrically with uncertainties less than 1%. Sky transmissionvariations were minimized via a system of synchronous polaroid rotationand bidirectional charge shifting. In all, 80 stars behind the peripheryof the globule were accurately analyzed polarimetrically. Thelarge-scale (1-2 pc) magnetic field direction around CB 4 was found tobe very uniform (P.A. = 63.3 deg +/- 1.1 deg). Double-Gaussian fittingof the polarization position angle histogram gave a dispersion of 10 degabout the primary field direction. Possible field-line compression wasfound inward of approximately 0.2 pc from the cloud center. Noappreciable twisting of field lines was found. By plotting stellarseparations against differences of polarization angles, CB 4 was foundto have a magnetic field decorrelation length of approximately 0.1 pc,similar to the size of the visually opaque cire, but much smaller thanthe size of the bright optical rim or CO half-power contour ofapproximately 0.5 pc. The magnetic field decorrelation length may berelated to a characteristic transient clumping size, or perhaps even toclumps of a more permanent nature.
| An Einstein Observatory SAO-based catalog of B-type stars
About 4000 X-ray images obtained with the Einstein Observatory are usedto measure the 0.16-4.0 keV emission from 1545 B-type SAO stars fallingin the about 10 percent of the sky surveyed with the IPC. Seventy-fourdetected X-ray sources with B-type stars are identified, and it isestimated that no more than 15 can be misidentified. Upper limits to theX-ray emission of the remaining stars are presented. In addition tosummarizing the X-ray measurements and giving other relevant opticaldata, the present extensive catalog discusses the reduction process andanalyzes selection effects associated with both SAO catalog completenessand IPC target selection procedures. It is concluded that X-rayemission, at the level of Lx not less than 10 exp 30 ergs/s, is quitecommon in B stars of early spectral types (B0-B3), regardless ofluminosity class, but that emission, at the same level, becomes lesscommon, or nonexistent, in later B-type stars.
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Pozíciós és asztrometriai adatok
| Csillagkép: | Ikrek |
| Rektaszcenzió: | 07h27m02.97s |
| Deklináció: | +16°05'58.0" |
| Vizuális fényesség: | 9.206 |
| RA sajátmozgás: | -0.7 |
| Dec sajátmozgás: | 0.6 |
| B-T magnitude: | 9.121 |
| V-T magnitude: | 9.199 |
Katalógusok és elnevezések:
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