11![HPOL: World’s Largest Database of Optical Spectropolarimetry M.R. Meade, B.L. Babler, B.A. Whitney, K.H. Nordsieck, K.S. Bjorkman, J.P. Wisniewski, A.M. Magalhaes, M.J. Wolff Stars with a V magnitude range of 0.1 to 12 HPOL: World’s Largest Database of Optical Spectropolarimetry M.R. Meade, B.L. Babler, B.A. Whitney, K.H. Nordsieck, K.S. Bjorkman, J.P. Wisniewski, A.M. Magalhaes, M.J. Wolff Stars with a V magnitude range of 0.1 to 12](https://www.pdfsearch.io/img/c030ad8fa78bda2bbd025f81c59a5f37.jpg) | Add to Reading ListSource URL: www.sal.wisc.eduLanguage: English - Date: 2011-08-10 16:44:10
|
---|
12![Effect of Chemical Solutions on the Strength Effect of Chemical Solutions on the Strength](https://www.pdfsearch.io/img/f879f185c14cec1e72b1b97c667d95cf.jpg) | Add to Reading ListSource URL: rockmechanics.curtin.edu.auLanguage: English - Date: 2012-07-05 21:30:57
|
---|
13![The Astrophysical Journal, 720:887–903, 2010 September 1 C[removed]doi:[removed]637X[removed] The Astrophysical Journal, 720:887–903, 2010 September 1 C[removed]doi:[removed]637X[removed]](https://www.pdfsearch.io/img/0a4d772241f2f85316f5b25e96bd4b2a.jpg) | Add to Reading ListSource URL: www.nrl.navy.milLanguage: English - Date: 2012-12-06 11:51:46
|
---|
14![Disk structure and dynamics in intermediate-mass Herbig Ae stars ´ ´m1 , A. Ko ´ spa ´l2 , A. Moo ´ r1 , M. Kun1 , Zs. Rega Disk structure and dynamics in intermediate-mass Herbig Ae stars ´ ´m1 , A. Ko ´ spa ´l2 , A. Moo ´ r1 , M. Kun1 , Zs. Rega](https://www.pdfsearch.io/img/1bcc23795687ff4af2168a08a688389f.jpg) | Add to Reading ListSource URL: keplerscience.arc.nasa.govLanguage: English - Date: 2014-08-23 20:45:00
|
---|
15![GLOSSARY
GLOSSARY* AGB star GLOSSARY
GLOSSARY* AGB star](https://www.pdfsearch.io/img/592d07429e7cc313b72e0be2ed7b8f22.jpg) | Add to Reading ListSource URL: www.uapress.arizona.eduLanguage: English - Date: 2007-04-05 13:30:42
|
---|
16![PROPERTIES AND EVOLUTION OF DISKS AROUND PRE-MAIN-SEQUENCE STARS OF INTERMEDIATE MASS ANTONELLA NATTA Osservatorio Astrofisico di Arcetri VLADIMIR P. GRININ PROPERTIES AND EVOLUTION OF DISKS AROUND PRE-MAIN-SEQUENCE STARS OF INTERMEDIATE MASS ANTONELLA NATTA Osservatorio Astrofisico di Arcetri VLADIMIR P. GRININ](https://www.pdfsearch.io/img/7ba80c684db4ea12b42e5c89bd4767f5.jpg) | Add to Reading ListSource URL: www.uapress.arizona.eduLanguage: English - Date: 2007-04-05 13:30:26
|
---|
17![Science Program Book for Fifth Spitzer Science Conference New Light on Young Stars: Spitzer’s View of Circumstellar Disks October[removed] Science Program Book for Fifth Spitzer Science Conference New Light on Young Stars: Spitzer’s View of Circumstellar Disks October[removed]](https://www.pdfsearch.io/img/a2a1ca710b32861ff0d94cf4e9c56a65.jpg) | Add to Reading ListSource URL: www.ipac.caltech.eduLanguage: English - Date: 2008-10-16 00:58:46
|
---|
18![The Astrophysical Journal, 779:178 (13pp), 2013 December 20 C[removed]doi:[removed]637X[removed] The Astrophysical Journal, 779:178 (13pp), 2013 December 20 C[removed]doi:[removed]637X[removed]](https://www.pdfsearch.io/img/48a4ebe9f0754b692521497b6f597bb0.jpg) | Add to Reading ListSource URL: www.nrl.navy.milLanguage: English - Date: 2014-01-10 16:11:51
|
---|
19![Abstract. Hα spectropolarimetry on Herbig Ae/Be stars shows that the innermost regions of intermediate mass (2 – 15 M⊙ ) Pre-Main Sequence stars are flattened. This may be the best evidence to date that the higher m Abstract. Hα spectropolarimetry on Herbig Ae/Be stars shows that the innermost regions of intermediate mass (2 – 15 M⊙ ) Pre-Main Sequence stars are flattened. This may be the best evidence to date that the higher m](https://www.pdfsearch.io/img/d7aba59ba937cd538ac17ad6fa77b12c.jpg) | Add to Reading ListSource URL: www.modern-medical-science.site88.netLanguage: English - Date: 2013-02-01 19:59:24
|
---|
20![arXiv:1302.7122v1 [astro-ph.GA] 28 Feb 2013 arXiv:1302.7122v1 [astro-ph.GA] 28 Feb 2013](https://www.pdfsearch.io/img/e1bb8dce150946d8c97febeb5eb0d864.jpg) | Add to Reading ListSource URL: arxiv.orgLanguage: English - Date: 2013-02-28 20:12:21
|
---|