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    31. SAO Summer Intern Program Projects, 1999
    ... We analyze photometric and spectroscopic observations of the supernova SN 1999by in the spiral galaxy NGC 2841. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects99.html -- 36.2 Кб -- 01.10.2012
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    32. http://hea-www.harvard.edu/XJET/references.html
    ... Keel, W.C., White, R.E., Owen, F.N., & Ledlow, M.J. 2006 AJ, 132 , 2233. ``The Spiral Host Galaxy of the Double Radio Source 0313-192'' . [ astro-ph | ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/XJET/references.html -- 84.2 Кб -- 27.02.2014
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    33. AAS HEAD 1997 Poster
    ... Observations of edge-on galaxies[ 3 , 10 , 19 ] have demonstrated that some have extended hot halos; while observations of face-on spiral galaxies[ 5 ] provide upper limits to emission from their halos. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~juda/sxrb/head97.html -- 46.5 Кб -- 01.10.2012
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    34. http://hea-www.harvard.edu/~bradw/cv/papers/whiteGenX.pdf
    ... But observations of nearby fac e-on spiral galaxies show that dozens of molecular clouds with 105 - 106 M producing clusters with 104 stars must be present in our Galaxy. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/whiteGenX.pdf -- 434.2 Кб -- 08.10.2009
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    35. http://hea-www.harvard.edu/~kim/pap/2014_N4649_AGNfeedback.pdf
    ... Its companion, located at 2.5 to the northwest, is the spiral galaxy NGC 4647. NGC 4649 harbors a faint nuclear radio source (Condon et al. 2002). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2014_N4649_AGNfeedback.pdf -- 1400.2 Кб -- 19.10.2014
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    36. http://hea-www.harvard.edu/~kim/pap/2005_ChaMP_hard_AGN.pdf
    ... To illustrate, we plot in Figure 6a the expected colors of an elliptical ( E0) and a spiral (Sb) galaxy using the Hyper_z ( Bolzonella et al. 2000) photometric code. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2005_ChaMP_hard_AGN.pdf -- 1020.4 Кб -- 06.12.2010
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    37. http://hea-www.harvard.edu/~kim/pap/2005_M33_I.pdf
    ... INTRODUCTION M33 is a late-type spiral galaxy, type Sc II ­ III, and the third ... type between the large early-type spiral galaxies ( Milky Way and M31) and the ... 1991) M33 is the second nearest spiral galaxy; it spans roughly 73 0 ; 45 0 on the ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2005_M33_I.pdf -- 431.8 Кб -- 06.12.2010
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    38. http://hea-www.harvard.edu/~kim/pap/2010_highlights_JD8.pdf
    ... galaxies, which are intermediate between ellipticals and spirals, are similar to elliptical galaxies in their optical spectra ... Nevertheless, S0's in the cluster environment may have been changed from spiral galaxies when falling into clusters. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2010_highlights_JD8.pdf -- 1082.1 Кб -- 06.12.2010
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    39. http://hea-www.harvard.edu/~pgreen/Papers/SDSS1254.pdf
    ... The matching experiment here only informs us that the progenitor spiral galaxies are required to be sufficiently large (i.e., scale length of the stellar disk Rdisk 4 kpc), to produce the length of the tidal tails, and that they must have contained pre ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/SDSS1254.pdf -- 1028.8 Кб -- 02.02.2010
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    40. http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.pdf
    ... The brightest nearby spiral galaxies observed by Fabbiano & Trinchieri (1985) show log L \ 23.5, and elliptical galaxies achieve log L \ 24, 2 keV is near to which keV the apparent X-ray luminosity2 of our 2 detected loBAL QSOs. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.pdf -- 161.6 Кб -- 14.09.2005
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