INSTRUCTION MANUAL
... NexStar hand control has built-in instructions to guide you through all the alignment procedures needed to have the telescope up and running in minutes. Use this manual in conjunction with the on-screen instructions provided by the hand control. The manual gives detailed information regarding each s ...
... NexStar hand control has built-in instructions to guide you through all the alignment procedures needed to have the telescope up and running in minutes. Use this manual in conjunction with the on-screen instructions provided by the hand control. The manual gives detailed information regarding each s ...
Comprehensive search for natural satellites of Vesta by the Dawn
... absence of satellites in the context of the impact and ejecta history of Vesta in the discussion. The mission’s approach phase included searching for satellites around Vesta for more than two months. During these sequences, Vesta was targeted on a regular basis and if there were a satellite, this wa ...
... absence of satellites in the context of the impact and ejecta history of Vesta in the discussion. The mission’s approach phase included searching for satellites around Vesta for more than two months. During these sequences, Vesta was targeted on a regular basis and if there were a satellite, this wa ...
LCM SerieS
... telescope! The LCM ushers in a whole new generation of computer automated technology. Simple and friendly to use, the LCM telescope is up and running after locating just three bright celestial objects. It’s the perfect combination of power and portability. If you are new to astronomy, you may wish t ...
... telescope! The LCM ushers in a whole new generation of computer automated technology. Simple and friendly to use, the LCM telescope is up and running after locating just three bright celestial objects. It’s the perfect combination of power and portability. If you are new to astronomy, you may wish t ...
T3-Cosmic Star Formation History
... formation of cosmic structure, and observations in this field have accumulated at an astonishing pace. Multiwavelength imaging surveys with the Hubble (HST) and Spitzer space telescopes and ground-based facilities, together with spectroscopic follow-up with 8-m-class telescopes, have led to the disco ...
... formation of cosmic structure, and observations in this field have accumulated at an astonishing pace. Multiwavelength imaging surveys with the Hubble (HST) and Spitzer space telescopes and ground-based facilities, together with spectroscopic follow-up with 8-m-class telescopes, have led to the disco ...
ALMA - ESO
... Detect the Milky Way at z=3 Measure dust broadband emission and spectral line radiation from atoms and molecules in high-z galaxies to obtain detailed morphology and kinematics ...
... Detect the Milky Way at z=3 Measure dust broadband emission and spectral line radiation from atoms and molecules in high-z galaxies to obtain detailed morphology and kinematics ...
arXiv:astro-ph/0701557v1 19 Jan 2007
... either: (a) been progressing at a constant rate for the past several 107 yr, but with few high-mass stars; or (b) been decaying exponentially since the onset of a burst 15 Myr ago, with a fairly ‘normal’ initial mass function (IMF). However, they were unable to assess the possible variation of the S ...
... either: (a) been progressing at a constant rate for the past several 107 yr, but with few high-mass stars; or (b) been decaying exponentially since the onset of a burst 15 Myr ago, with a fairly ‘normal’ initial mass function (IMF). However, they were unable to assess the possible variation of the S ...
THE PERIOD OF ROTATION OF THE SUN
... instrument, and has three separately tunable receivers (400-1600 MHz) which record data digitally and can display the data as a chart record or as sound. VIREO simulates modern astronomical observation by accessing a number of databases, both on-line and in data files provided with the software. The ...
... instrument, and has three separately tunable receivers (400-1600 MHz) which record data digitally and can display the data as a chart record or as sound. VIREO simulates modern astronomical observation by accessing a number of databases, both on-line and in data files provided with the software. The ...
Elements of astronomy
... Great care has been taken to render every statement clear and precise, and it is important that the student, in his recitations, should be trained to a similar pre- ...
... Great care has been taken to render every statement clear and precise, and it is important that the student, in his recitations, should be trained to a similar pre- ...
Slide 1
... Moving Towards Black Holes • If the remaining neutron star has a “critical mass” (about 3MSun) it can continue to collapse • Nothing left to oppose the crush of gravity! Continues to collapse until it becomes a Black ...
... Moving Towards Black Holes • If the remaining neutron star has a “critical mass” (about 3MSun) it can continue to collapse • Nothing left to oppose the crush of gravity! Continues to collapse until it becomes a Black ...
View
... of the most sophisticated and easy to use telescopes available on the market today. Take time to read through this manual before embarking on your journey through the Universe. It may take a few observing sessions to become familiar with your telescope, so you should keep this manual handy until you ...
... of the most sophisticated and easy to use telescopes available on the market today. Take time to read through this manual before embarking on your journey through the Universe. It may take a few observing sessions to become familiar with your telescope, so you should keep this manual handy until you ...
G030515-00 - DCC
... indicate some asymmetry present •Simulations do not succeed from initiation to explosions LIGO-G030515-00-W ...
... indicate some asymmetry present •Simulations do not succeed from initiation to explosions LIGO-G030515-00-W ...
The SMC as a probe of dust in the early Universe
... fundamentally different dust chemistries in high-redshift galaxies, showing emission from polycyclic aromatic hydrocarbons (PAHs) at z = 3.0 (Huang et al. 2007), amorphous silicate emission at z = 2.3 (Teplitz et al. 2006), crystalline silicates out to z = 0.3 (Spoon et al. 2006), and even the possi ...
... fundamentally different dust chemistries in high-redshift galaxies, showing emission from polycyclic aromatic hydrocarbons (PAHs) at z = 3.0 (Huang et al. 2007), amorphous silicate emission at z = 2.3 (Teplitz et al. 2006), crystalline silicates out to z = 0.3 (Spoon et al. 2006), and even the possi ...
9 The Clearing of Protoplanetary Disks and of the Protosolar Nebula
... a few to 10 Myr to form Jupiter-like planets at 5 AU (see, e.g. Lissauer & Stevenson 2007), meaning that primordial gas should persist for as long in the disk. Whether terrestrial planets can form and whether their orbits will be circular as those of Earth and Venus strongly depend on the amount of ...
... a few to 10 Myr to form Jupiter-like planets at 5 AU (see, e.g. Lissauer & Stevenson 2007), meaning that primordial gas should persist for as long in the disk. Whether terrestrial planets can form and whether their orbits will be circular as those of Earth and Venus strongly depend on the amount of ...
The Life Cycle of Stars: Supernovae in Starbursts by Jason Kezwer
... with a K-band peak of approximately ∆mK = 0.16 magnitudes. To find the true ...
... with a K-band peak of approximately ∆mK = 0.16 magnitudes. To find the true ...
The evolution of low-metallicity massive stars - Argelander
... To understand their behaviors and the ways they interact with their environments, however, we would optimally need data of a large number of them with the same age at known distance, preferably in the local Universe, so constraints on their evolution could be obtained. It is imperative to know the d ...
... To understand their behaviors and the ways they interact with their environments, however, we would optimally need data of a large number of them with the same age at known distance, preferably in the local Universe, so constraints on their evolution could be obtained. It is imperative to know the d ...
PDF 523 KB
... for his observations of Mars ). He founded his private observatory in 1894 in Flagstaff Arizona, and dedicated portion of his life searching for the planet beyond Neptune. A few times he was very close to finalizing his ultimate dream. It looks like a few times PLuto was missed. It is very sad that ...
... for his observations of Mars ). He founded his private observatory in 1894 in Flagstaff Arizona, and dedicated portion of his life searching for the planet beyond Neptune. A few times he was very close to finalizing his ultimate dream. It looks like a few times PLuto was missed. It is very sad that ...
Spitzer Spectroscopy of Circumstellar Disks in the 5 Myr Old Upper
... µm. These results imply that the mechanisms responsible for disk dispersal operate more efficiently for high mass stars than for their low-mass counterparts. Consequently, longer timescales may be available for the buildup of planetesimals and planetary systems within the terrestrial zone for stars ...
... µm. These results imply that the mechanisms responsible for disk dispersal operate more efficiently for high mass stars than for their low-mass counterparts. Consequently, longer timescales may be available for the buildup of planetesimals and planetary systems within the terrestrial zone for stars ...
The Circumstellar Environments of Young Stars at AU Scales
... emission (Millan-Gabet et al., 1999). The measured size was unexpectedly large in the context of then-current disk models of HAeBe objects (e.g., Hillenbrand et al., 1992), which predicted NIR diameter of 0.2 AU based on optically thick, geometrically thin circumstellar disks with a small dust-free ...
... emission (Millan-Gabet et al., 1999). The measured size was unexpectedly large in the context of then-current disk models of HAeBe objects (e.g., Hillenbrand et al., 1992), which predicted NIR diameter of 0.2 AU based on optically thick, geometrically thin circumstellar disks with a small dust-free ...