Presentation is loading. Please wait.

Presentation is loading. Please wait.

Distant Galaxies Hubble Space Telescope Ultra Deep Field.

Published byKatrina Stewart Modified over 8 years ago

Similar presentations

Presentation on theme: "Distant Galaxies Hubble Space Telescope Ultra Deep Field."— Presentation transcript:

1 Distant Galaxies Hubble Space Telescope Ultra Deep Field

2 Leo Triplet (APOD 2006 March 9) NGC 3628 M 66 M 65

3 M 101

4 NGC 891

5 A Very Nearby Edge-On Spiral Galaxy Our Own Milky Way!

6 Optical Dust and Molecular Clouds

7 Neutral Atomic Gas (hydrogen 21 cm line)

8 Ionized Gas (74 cm, mostly nonthermal)

9 The Optical Milky Way

10 Neutral Atomic Gas (hydrogen 21cm line)

11 Hot Ionized Gas (soft X-rays, 4.96 nm) Local Bubble + Extragalactic Background

12 Hot Ionized Gas (soft X-rays, 1.65 nm) Nearby Bubbles + SNRs + Galactic Core, with some extinction

13 Hot Ionized Gas (soft X-rays, 0.827 nm) Nearby Bubbles + SNRs + Galactic Core, with less extinction

14 Hot Ionized Gas (soft X-rays, 3 bands)

15 Ionized Gas (74 cm, unpolarized)

16 Ionized Gas + Magnetic Fields (21 cm, polarized)

Download ppt "Distant Galaxies Hubble Space Telescope Ultra Deep Field."

Similar presentations

Ming Zhu (JAC/NRC) P. P. Papadopoulos (Argelander Institute for Astronomy, Germany) Yu Gao (Purple Mountain Observatory, China) Ernie R. Seaquist (U. of.

Ming Zhu (JAC/NRC) P. P. Papadopoulos (Argelander Institute for Astronomy, Germany) Yu Gao (Purple Mountain Observatory, China) Ernie R. Seaquist (U. of.
Galaxies-I. By the 1700’s the old notion that the Earth was the center of the Universe was overthrown by the success of Newton’s theory of universal gravitation,

Galaxies-I. By the 1700’s the old notion that the Earth was the center of the Universe was overthrown by the success of Newton’s theory of universal gravitation,
Chapter 15 The Milky Way Galaxy.

Chapter 15 The Milky Way Galaxy.
14.2 Galactic Recycling Our Goals for Learning How does our galaxy recycle gas into stars? Where do stars tend to form in our galaxy?

14.2 Galactic Recycling Our Goals for Learning How does our galaxy recycle gas into stars? Where do stars tend to form in our galaxy?
A105 Stars and Galaxies  Milky Way Homework (#11) due today  Projects Due Nov. 30  For next week: Units 74, 75, 76, 78, 79  “rooftop” tonight, 8 PM,

A105 Stars and Galaxies  Milky Way Homework (#11) due today  Projects Due Nov. 30  For next week: Units 74, 75, 76, 78, 79  “rooftop” tonight, 8 PM,
© 2010 Pearson Education, Inc. The Milky Way. © 2010 Pearson Education, Inc. Dusty gas clouds obscure our view because they absorb visible light. This.

© 2010 Pearson Education, Inc. The Milky Way. © 2010 Pearson Education, Inc. Dusty gas clouds obscure our view because they absorb visible light. This.
X-ray Astronomy. The astmosphere is opaque to X- rays (good thing, too!)

X-ray Astronomy. The astmosphere is opaque to X- rays (good thing, too!)
The Milky Way Galaxy Chapter 15. The Milky Way Almost everything we see in the night sky belongs to the Milky Way We see most of the Milky Way as a faint.

The Milky Way Galaxy Chapter 15. The Milky Way Almost everything we see in the night sky belongs to the Milky Way We see most of the Milky Way as a faint.
The Interstellar Medium (ISM): The Birth of Stars.

The Interstellar Medium (ISM): The Birth of Stars.
General Astronomy The Interstellar Medium Credits: Much of this slideset is modified from lectures by Dr. Peter Newbury (UBC)

General Astronomy The Interstellar Medium Credits: Much of this slideset is modified from lectures by Dr. Peter Newbury (UBC)
Measuring the Gas in Galaxies in the Distant Past Philip Lah Too late. Here comes the SKA.

Measuring the Gas in Galaxies in the Distant Past Philip Lah Too late. Here comes the SKA.
Multiwavelength Sky by NASA. Radio Continuum (408 MHz). Intensity of radio continuum emission from surveys with ground- based radio telescopes (Jodrell.

Multiwavelength Sky by NASA. Radio Continuum (408 MHz). Intensity of radio continuum emission from surveys with ground- based radio telescopes (Jodrell.
Lecture Outline Chapter 15: Our Galaxy © 2015 Pearson Education, Inc.

Lecture Outline Chapter 15: Our Galaxy © 2015 Pearson Education, Inc.
QUASARS Monsters of the ancient Universe Professor Jill Bechtold Steward Observatory Tucson Amateur Astronomers, Dec. 6, 2002.

QUASARS Monsters of the ancient Universe Professor Jill Bechtold Steward Observatory Tucson Amateur Astronomers, Dec. 6, 2002.
Galaxies Astronomy 315 Professor Lee Carkner Lecture 20.

Galaxies Astronomy 315 Professor Lee Carkner Lecture 20.
The Interstellar Medium Astronomy 315 Professor Lee Carkner Lecture 19.

The Interstellar Medium Astronomy 315 Professor Lee Carkner Lecture 19.
14 Galaxies Island Universes. 14 Copyright – FORS1 VLTI, European Southern Observatory.

14 Galaxies Island Universes. 14 Copyright – FORS1 VLTI, European Southern Observatory.
The Formation of Stars Chapter 11. Giant Molecular Clouds Large Low density Cold To Form Stars Small High density Hot.

The Formation of Stars Chapter 11. Giant Molecular Clouds Large Low density Cold To Form Stars Small High density Hot.
Agenda: galaxies The Milky Way Types of galaxies Finding distances to galaxies.

Agenda: galaxies The Milky Way Types of galaxies Finding distances to galaxies.
Taking the fingerprints of stars, galaxies, and interstellar gas clouds Absorption and emission from atoms, ions, and molecules.

Taking the fingerprints of stars, galaxies, and interstellar gas clouds Absorption and emission from atoms, ions, and molecules.

Similar presentations

Ads by Google