Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Hakobian, Nicholas S."'
Autor:
Hull, Charles L. H., Plambeck, Richard L., Kwon, Woojin, Bower, Geoffrey C., Carpenter, John M., Crutcher, Richard M., Fiege, Jason D., Franzmann, Erica, Hakobian, Nicholas S., Heiles, Carl, Houde, Martin, Hughes, A. Meredith, Lamb, James W., Looney, Leslie W., Marrone, Daniel P., Matthews, Brenda C., Pillai, Thushara, Pound, Marc W., Rahman, Nurur, Sandell, Göran, Stephens, Ian W., Tobin, John J., Vaillancourt, John E., Volgenau, N. H., Wright, Melvyn C. H.
We present {\lambda}1.3 mm CARMA observations of dust polarization toward 30 star-forming cores and 8 star-forming regions from the TADPOL survey. We show maps of all sources, and compare the ~2.5" resolution TADPOL maps with ~20" resolution polariza
Externí odkaz:
http://arxiv.org/abs/1310.6653
Autor:
Hull, Charles L. H., Plambeck, Richard L., Bolatto, Alberto D., Bower, Geoffrey C., Carpenter, John M., Crutcher, Richard M., Fiege, Jason D., Franzmann, Erica, Hakobian, Nicholas S., Heiles, Carl, Houde, Martin, Hughes, A. Meredith, Jameson, Katherine, Kwon, Woojin, Lamb, James W., Looney, Leslie W., Matthews, Brenda C., Mundy, Lee, Pillai, Thushara, Pound, Marc W., Stephens, Ian W., Tobin, John J., Vaillancourt, John E., Volgenau, N. H., Wright, Melvyn C. H.
Publikováno v:
2013 ApJ, 768, 159
We present results of 1.3 mm dust polarization observations toward 16 nearby, low-mass protostars, mapped with ~2.5" resolution at CARMA. The results show that magnetic fields in protostellar cores on scales of ~1000 AU are not tightly aligned with o
Externí odkaz:
http://arxiv.org/abs/1212.0540
A previously unseen maser in the J = 1 - 0 transition of HCO$^+$ has been detected by the Combined Array for Millimeter-wave Astronomy (CARMA). A sub-arcsecond map was produced of the 2 arcmin$^2$ region around DR21(OH), which has had previous detect
Externí odkaz:
http://arxiv.org/abs/1209.2092
We have carried out a multi-species study of a region which has had previous measurements of strong magnetic fields through the CN Zeeman effect in order to to explore the relationship between CN and N$_2$H$^+$, both of which have evidence that they
Externí odkaz:
http://arxiv.org/abs/1103.3082
Akademický článek
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Akademický článek
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Publikováno v:
Astrophysical Journal Letters; 10/10/2012, Vol. 758 Issue 1, Special section p1-4, 4p
