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На этой странице приведены все страницы сервера www.vsop.isas.ac.jp ,которые мы индексируем. Показаны документы 461 - 477 из 477.

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461. source comment

. Comment on J0334-4008 . Our image is not consistent with the one at 5 GHz by Shen et al. (1998) which shows an extension in the opposite direction to that seen in our image. A redshift of 1.445 is widely quoted for this source, but there is little to support this value. Drinkwater et al. (1997) were unable to measure a redshift for this source. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0334-4008.comment.htm -- 1.6 Кб -- 16.10.2000
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462. source comment

. Comment on J0322-3712 . No detction: not surprising in view of the very low flux density of the compact core of this source, <4 mJy, from the observation by Morganti et al. (1997) using the 275 km Parkes-Tidbinbilla interferometer at 2.3 GHz. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0322-3712.comment.htm -- 1.5 Кб -- 16.10.2000
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463. source comment

. Comment on J0319+4130 . Our image does represent the main source structure. However, due to the limited u-v coverage, it does not have as high fidelity as other known images, such as the one at 5 GHz by Romney et al. (1995). VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0319+4130.comment.htm -- 1.5 Кб -- 16.10.2000
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464. source comment

. Comment on J0318+4151 . No detection: according to global VLBI observations at 5 GHz by Xu, O'Dea & Biretta (1999), the core of this double-tail radio galaxy has a brightness of 13 mJy/beam, too weak for us to be detected. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0318+4151.comment.htm -- 1.5 Кб -- 16.10.2000
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465. source comment

. Comment on J0241-0815 . Our image agrees well with that reported by Kellermann et al. (1999). VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0241-0815.comment.htm -- 1.4 Кб -- 16.10.2000
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466. source comment

. Comment on J0238+1636 . Our data show that in June 1996 the source had an unusually low flux density with an angular size of 0.6". The source is usually highly variable, strong and extremely compact. However, Chen, Zhang & Sjouwerman (1999) also claim the source was resolved with EVN observations at 5 GHz about 8 months after our observation when the flux density was still unusually low. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0238+1636.comment.htm -- 1.7 Кб -- 16.10.2000
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467. source comment

. Comment on J0226+3421 . A Compact Steep Spectrum (CSS) source observed with the European VLBI Network (EVN) (Dallacasa et al. (1995) and references therein). Recent redshift measurement by Willott et al. (1998). VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0226+3421.comment.htm -- 1.5 Кб -- 16.10.2000
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468. source comment

. Comment on J0221+3556 . A gravitational lens; the two lensed components are shown in Figure 4. See Polatidis et al. (1995) and Xu et al. (1995) for other VLBI images at 1.6 and 5 GHz, respectively. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0221+3556.comment.htm -- 1.5 Кб -- 16.10.2000
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469. source comment

. Comment on J0137+3309 . Resolved: a source with known arc-second structure and too resolved to be imaged here. The shortest VLBA baselines detect about 0.8 Jy from the source. See Figure 3. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0137+3309.comment.htm -- 1.5 Кб -- 16.10.2000
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470. source comment

. Comment on J0126-0123 . No detection: this object has been studied with the Molonglo telescope at 408 MHz (Schilizzi & McAdam 1975) as a source with a size between 2 and 5 . It is near an Abell cluster (Owen & Ledlow 1997). The data could be confused with a strong radio source (3C 40) identified with a pair of galaxies at z=0.018, 170" from our field center. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0126-0123.comment.htm -- 1.7 Кб -- 16.10.2000
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471. source comment

. Comment on J0120-2701 . A VLBI image at 5 GHz is published by Shen et al. (1998). Their centrally symmetric S-shape structure is not confirmed from our image. It is a prominent radio and X-ray source. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0120-2701.comment.htm -- 1.5 Кб -- 16.10.2000
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472. source comment

. Comment on J0119+3210 . The source is well resolved, and the image is somewhat consistent with the 2.3 GHz image from the USNO database. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0119+3210.comment.htm -- 1.4 Кб -- 16.10.2000
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473. source comment

. Comment on J0119+0829 . Our image is in good agreement with the 1.6 and 5 GHz VLBA images of Cohen et al. (1997). VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0119+0829.comment.htm -- 1.4 Кб -- 16.10.2000
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474. source comment

. Comment on J0042+2320 . 8.4 GHz VLBI image from the USNO database shows a N-NE extension of 4 mas which is not visible in our image due to the lack of resolution in that direction. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0042+2320.comment.htm -- 1.5 Кб -- 16.10.2000
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475. source comment

. Comment on J0029+3456 . The redshift value of 0.600 in Table 1 is from Hutchings et al. (1994). R.C. Vermeulen (2000, private communication) gives z=0.517. VLBApls home page . Last modified: 16 Oct 2000

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0029+3456.comment.htm -- 1.4 Кб -- 16.10.2000
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476. VSOP Symposium Proceedings

Individual papers from the VSOP Symposium Proceedings, "Astrophysical Phenomena Revealed by Space VLBI", eds H. Hirabayashi, P.G. Edwards and D.W. Murphy (ISAS), can be downloaded as gzipped postscript files by clicking on the links below. ... Multi-Epoch Global+VSOP/HALCA Observations of Virgo A at lambda 6 cm . ... Space-VLBI Observations of the Core-Jet in the Nearby Spiral Galaxy M81 . ... H. Hirabayashi, P.G. Edwards, B.G. Piner et al. ... Pentachromatic VSOP and VLBA Survey of GPS Sources . ...

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/vsopsymp/papers/index.html -- 12.2 Кб -- 23.08.2000
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477. Big Antenna

[ Сохраненная копия ] Ссылки http://www.vsop.isas.ac.jp/bigant.html -- 1.4 Кб -- 07.12.1998
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