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Local tests of spatial variation of m e /m p

Local tests of spatial variation of m e /m p

Local tests of spatial variation of m e /m p. S. A. Levshakov Department of Theoretical Astrophysics Physical-Technical Institute, St. Petersburg. JINR, Dec 1-5, 2014. Department of Theoretical Astrophysics Physical-Technical Institute, St. Petersburg , 201. Low energies.

By johana
(428 views)

W4 West(AFGL 333) 領域におけるアンモニア分子輝線観測

W4 West(AFGL 333) 領域におけるアンモニア分子輝線観測

W4 West(AFGL 333) 領域におけるアンモニア分子輝線観測. 副島隆史 ( 大分大学 M2) 仲野誠(大分大学) 面高俊宏 , 半田利弘 , 亀﨑達也 , Ross Burns, 馬場達也 , 松尾光洋 , 宮崎竜之介 , 吉田友哉(鹿児島大学) 永山匠 , 砂田和良 , James Chibueze , 久野成夫( NAOJ ). 31th NRO Users Meeting (2013). Introduction. W3 Main. W4.

By duscha
(148 views)

Mopra Induction Weekend May 2005

Mopra Induction Weekend May 2005

Determination of physical properties from molecular lines Kate Brooks Australia Telescope National Facility. Mopra Induction Weekend May 2005. Interstellar Molecules. Ehrenfreund & Charnley 2000, ARA&A, 38, 427.

By diallo
(111 views)

Chapter 1 Answers

Chapter 1 Answers

Chapter 1 Answers. #8 3.05mL the 2.87mL grad cyl measurement limits precision #28 examples of matter/mixtures and phys/chem change #32 sig figs 1,2,3,3,2,3,3,4 #33 rounding 0.000342, 10340, 17.992, 337000 #37 188.1, 12, 4x10 -7 , 6.3x10 -25 , 4.90 , 0.22%

By gavivi
(168 views)

Drill: Calculate the pH of 0.10 M H 2 Z in 0.50 M KHZ. K a1 = 2.0 x 10 -5 K a2 = 5.0 x 10 -9

Drill: Calculate the pH of 0.10 M H 2 Z in 0.50 M KHZ. K a1 = 2.0 x 10 -5 K a2 = 5.0 x 10 -9

Drill: Calculate the pH of 0.10 M H 2 Z in 0.50 M KHZ. K a1 = 2.0 x 10 -5 K a2 = 5.0 x 10 -9. Hydrolysis Reactions. Hydrolysis. Any reaction in which water is decomposed with all or part of its decomposition portions combining with the products. Hydrolysis.

By coye
(148 views)

Allen et al. (2005)

Allen et al. (2005)

Johnstone et al. (2000). Allen et al. (2005). Tracing Dense Core Structure with NH 3. Oph B2. NH 3 (1,1) int. intensity (GBT). 850 m m continuum (JCMT). NH 3 emission shows excellent (but not perfect) correspondence with dust continuum emission. Tracing Dense Core Structure with NH 3.

By mingan
(216 views)

Acids and Bases

Acids and Bases

Acids and Bases. Three Definitions. Arrhenius acid – produces H + in soln base – produces OH - in soln Bronsted-Lowry acid – H + donor base – H + acceptor Lewis acid – electron pair acceptor base – electron pair donor. Conjugate acid-base pairs.

By tan
(173 views)

Chapter 4

Chapter 4

Chapter 4. Chemical Reactions. Changing Matter. Chemistry is defined as the study of matter and changes it undergoes. In chemistry, we recognize two different types of ways that matter can change. Physical Change Chemical Change. Physical Changes.

By hashim-davis
(55 views)

Allen et al. (2005)

Allen et al. (2005)

Johnstone et al. (2000). Allen et al. (2005). Tracing Dense Core Structure with NH 3. Oph B2. NH 3 (1,1) int. intensity (GBT). 850 m m continuum (JCMT). NH 3 emission shows excellent (but not perfect) correspondence with dust continuum emission. Tracing Dense Core Structure with NH 3.

By ulysses-blackwell
(121 views)

Glen Langston Astrobiology Review Green Bank Discoveries What Radio Astronomers Observe

Glen Langston Astrobiology Review Green Bank Discoveries What Radio Astronomers Observe

Signs of Life: Pre-biotic Chemistry New Discoveries with the NRAO 100m Diameter Green Bank Telescope (GBT). Glen Langston Astrobiology Review Green Bank Discoveries What Radio Astronomers Observe Future Directions. NRAO. glangsto@nrao.edu. Astrobiology. Credit: Pascal Ehrenfreund.

By sade-snyder
(81 views)

Drill: Calculate the pH of 0.10 M H 2 Z in 0.50 M KHZ. K a1 = 2.0 x 10 -5 K a2 = 5.0 x 10 -9

Drill: Calculate the pH of 0.10 M H 2 Z in 0.50 M KHZ. K a1 = 2.0 x 10 -5 K a2 = 5.0 x 10 -9

Drill: Calculate the pH of 0.10 M H 2 Z in 0.50 M KHZ. K a1 = 2.0 x 10 -5 K a2 = 5.0 x 10 -9. Hydrolysis Reactions. Hydrolysis. Any reaction in which water is decomposed with all or part of its decomposition portions combining with the products. Hydrolysis.

By caleb-bauer
(85 views)

Star Formation with the SKA

Star Formation with the SKA

Star Formation with the SKA. HII Region RCW 38 (VLT & ATCA). Tyler Bourke - Harvard-Smithsonian CfA. Star Formation with the SKA. What we know (or think we know) What we don't know, but would really like to What the SKA can do for Star Formation Studies

By heulwen-evans
(183 views)

What does Ammonia trace in Egg Nebula

What does Ammonia trace in Egg Nebula

What does Ammonia trace in Egg Nebula. Pao-Jan Chiu With Jeremy Lim 2003 8.27. Outline. Optical Structure of the Egg Nebula 12 CO Molecular Outflows Structure of NH 3 (1,1) Observations with VLA Results and Discussion Summary. CRL2688 - Egg Nebula. Proto-Planetary nebula (PPN)

By clinton-gomez
(95 views)

Chapter 4

Chapter 4

Chapter 4. Chemical Reactions. Changing Matter. Chemistry is defined as the study of matter and changes it undergoes. In chemistry, we recognize two different types of ways that matter can change. Physical Change Chemical Change. Physical Changes.

By bchapman
(2 views)

Alexander V. Lapinov , G.Yu.Golubiatnikov

Alexander V. Lapinov , G.Yu.Golubiatnikov

The real discovery is not to discover new lands, but to see the world with new eyes Marcel Proust (Ray Jayawardhana). The use of precise molecular line spectroscopy in a search for m e /m p variations. Alexander V. Lapinov , G.Yu.Golubiatnikov

By gtamara
(0 views)


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